Relevant bibliographies by topics / Stellar feedbacks

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Stellar feedbacks'

Author: Grafiati
Published: 8 June 2024
Last updated: 19 July 2025

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Journal articles on the topic "Stellar feedbacks"

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Ciardi, B. "Inhomogeneous reionization regulated by radiative and stellar feedbacks." Astronomical & Astrophysical Transactions 20, no. 1 (2001): 177–82. http://dx.doi.org/10.1080/10556790108208210.

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Ekström, Sylvia, Georges Meynet, Cyril Georgy, José Groh, Arthur Choplin, and Hanfeng Song. "Massive star evolution: feedbacks in low-Z environment." Proceedings of the International Astronomical Union 14, S344 (2018): 153–60. http://dx.doi.org/10.1017/s1743921318007238.

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AbstractMassive stars are the drivers of the chemical evolution of dwarf galaxies. We review here the basics of massive star evolution and the specificities of stellar evolution in low-Z environment. We discuss nucleosynthetic aspects and what observations could constrain our view on the first generations of stars.
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Ciardi, B., A. Ferrara, F. Governato, and A. Jenkins. "Inhomogeneous reionization of the intergalactic medium regulated by radiative and stellar feedbacks." Monthly Notices of the Royal Astronomical Society 314, no. 3 (2000): 611–29. http://dx.doi.org/10.1046/j.1365-8711.2000.03365.x.

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Dekel, Avishai, Nir Mandelker, Frederic Bournaud, Daniel Ceverino, Yicheng Guo, and Joel Primack. "Clump survival and migration in VDI galaxies: an analytical model versus simulations and observations." Monthly Notices of the Royal Astronomical Society 511, no. 1 (2022): 316–40. http://dx.doi.org/10.1093/mnras/stab3810.

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ABSTRACT We address the nature of the giant clumps in high-z galaxies that undergo violent disc instability, distinguishing between long-lived and short-lived clumps. We study the evolution of long-lived clumps during migration through the disc via an analytical model tested by simulations and confront theory with CANDELS-HST observations. The clump ‘bathtub’ model, which considers gas and stellar gain and loss, involves four parameters: the accretion efficiency α, the star formation rate (SFR) efficiency ϵd, and the outflow mass-loading factors for gas and stars, η and ηs. The corresponding t
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Fan, Bowen, Da Yang, and Dorian S. Abbot. "Climate Bistability at the Inner Edge of the Habitable Zone due to Runaway Greenhouse and Cloud Feedbacks." Astrophysical Journal Letters 973, no. 1 (2024): L22. http://dx.doi.org/10.3847/2041-8213/ad7789.

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Abstract Understanding the climate dynamics at the inner edge of the habitable zone is crucial for predicting the habitability of rocky exoplanets. Previous studies using global climate models (GCMs) have indicated that planets receiving high stellar flux can exhibit climate bifurcations, leading to bistability between a cold (temperate) and a hot (runaway) climate. However, the mechanism causing this bistability has not been fully explained, in part due to the difficulty associated with inferring mechanisms from small numbers of expensive numerical simulations in GCMs. In this study, we emplo
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Locci, Daniele, Antonino Petralia, Giuseppina Micela, Antonio Maggio, Angela Ciaravella, and Cesare Cecchi-Pestellini. "Extreme-ultraviolet- and X-Ray-driven Photochemistry of Gaseous Exoplanets." Planetary Science Journal 3, no. 1 (2022): 1. http://dx.doi.org/10.3847/psj/ac3f3c.

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Abstract The interaction of exoplanets with their host stars causes a vast diversity in bulk and atmospheric compositions and physical and chemical conditions. Stellar radiation, especially at the shorter wavelengths, drives the chemistry in the upper atmospheric layers of close orbiting gaseous giants, providing drastic departures from equilibrium. In this study, we aim at unfolding the effects caused by photons in different spectral bands on the atmospheric chemistry. This task is particularly difficult because the characteristics of chemical evolution emerge from many feedbacks on a wide ra
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Velmani, Premvijay, and Aseem Paranjape. "The evolving role of astrophysical modelling in dark matter halo relaxation response." Journal of Cosmology and Astroparticle Physics 2025, no. 07 (2025): 026. https://doi.org/10.1088/1475-7516/2025/07/026.

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Abstract We study the change in the radial distribution of dark matter within haloes in response to baryonic astrophysical processes in galaxies at different epochs, investigating the role of astrophysical modeling in cosmological hydrodynamic simulations in producing the response. We find that the linear quasi-adiabatic relaxation with additional dependence on the halo-centric distance provides a good description not only at z = 0, but also at an earlier epoch (z = 1) in the IllustrisTNG simulation suite, with parameters being more universal across a much larger variety of haloes at z = 1 tha
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Wang 王, Jing 菁., Xuchen 旭辰 Lin 林, Lister Staveley-Smith, et al. "FEASTS Combined with Interferometry. II. Significantly Changed H i Surface Densities and Even More Inefficient Star Formation in Galaxy Outer Disks." Astrophysical Journal 973, no. 1 (2024): 15. http://dx.doi.org/10.3847/1538-4357/ad6763.

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Abstract We update the H i surface density measurements for a subset of 17 THINGS galaxies by dealing with the short-spacing problem of the original Very Large Array (VLA) H i images. It is the same sample that Bigiel et al. used to study the relation between H i surface densities and star formation (SF) rate surface densities in galaxy outer disks, which are beyond the optical radius r 25. For 10 galaxies, the update is based on combining original THINGS VLA H i images with H i images taken by the single-dish FAST in the FEASTS program. The median increment of H i surface densities in outer d
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Fierlinger, Katharina M., Andreas Burkert, Evangelia Ntormousi, et al. "Stellar feedback efficiencies: supernovae versus stellar winds." Monthly Notices of the Royal Astronomical Society 456, no. 1 (2015): 710–30. http://dx.doi.org/10.1093/mnras/stv2699.

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D'Antona, Francesca. "Stellar evolution and feedback connections to stellar dynamics." Proceedings of the International Astronomical Union 2, no. 14 (2006): 430–31. http://dx.doi.org/10.1017/s1743921307011222.

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AbstractUntil a few years ago, the common paradigm for the formation of Globular Clusters (GCs) was that they constitute a ‘simple stellar population’ in which all the stars were formed from a chemically homogeneous cluster medium within a relatively short interval of time, at the beginning of the galactic life. In recent years, the spectroscopic information on the low luminosity (turnoff) cluster stars have extended to the unevolved stars the recognition that chemical anomalies are a common feature of GCs and not an exception. This has provoked a revolution in the simple view of GC formation,
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Dissertations / Theses on the topic "Stellar feedbacks"

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Maillard, Vincent. "Modèle des fronts de photoevaporation dans les régions de formation d'étoiles." Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO003.

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Les conditions de formation des étoiles est un sujet central en astrophysique. Le taux de formation stellaire (SFR) est relié à la masse de gaz moléculaire par la relation de Schmidt-Kennicutt. Une étoile modifie son nuage parent grâce aux vents, jets et à son rayonnement, balayant son environnement, détruisant des sites de formation d’étoiles, mais pouvant aussi en compresser et déstabiliser, déclenchant la formation de nouvelles étoiles. Ma thèse s’est concentrée sur la rétroaction radiative, largement dominée par celle des étoiles massives. Cela crée une région ionisée en expansion au plus
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Rogers, Hazel Claire. "Feedback from winds and supernovae in massive stellar clusters." Thesis, University of Leeds, 2013. http://etheses.whiterose.ac.uk/6858/.

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This thesis contains a study of the mechanical feedback from winds and supernovae on inhomogeneous molecular material left over from the formation of a massive stellar cluster. Firstly, the mechanical input from a cluster with three massive O-stars into a giant molecular cloud (GMC) clump containing 3240M⊙ of molecular material within a 4 pc radius is investigated using a 3D hydrodynamcial model. The cluster wind blows out of the molecular clump along low-density channels, into which denser clump material is entrained. The densest regions are surprisingly resistant to ablation by the cluster w
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Giarrusso, Daniele. "Properties of the galactic-scale gas circulation generated by stellar feedback." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20942/.

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Questo lavoro di tesi si propone di esaminare la simulazione di una galassia isolata simile alla Via Lattea e, in particolare, di analizzare i processi di feedback dovuto ad esplosioni di supernove, il meccanismo responsabile della generazione di outflow gassosi dal disco. Scopo della tesi è quello di testare la validità dei risultati ottenuti dalla simulazione (generata dal recente modello di feedback SMUGGLE presente nel codice a griglia mobile AREPO) dal punto di vista della formazione stellare, del tasso di esplosioni di supernove e dei fenomeni di outflow di gas su scala galattica. Sono
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Rey, Raposo Ramon. "The interplay between stellar feedback and galactic environment in molecular clouds." Thesis, University of Exeter, 2015. http://hdl.handle.net/10871/21022.

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In this thesis we address the problem of understanding the star formation process in giant molecular clouds in a galactic context. Most simulations of molecular clouds to date use an oversimplified set of initial conditions (turbulent spheres/boxes or colliding flows). Full galactic scale models are able to generate molecular clouds with complex morphologies and velocity fields but they fail to reproduce in detail the effects that occur at sub-pc scales (e.g. stellar feedback). Our goal is to build the bridge between these two scenarios, and to model the star formation process in molecular clo
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Smith, Matthew Carey. "Modelling star formation and stellar feedback in numerical simulations of galaxy formation." Thesis, University of Cambridge, 2018. https://www.repository.cam.ac.uk/handle/1810/277830.

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Remarkable progress has been made over the last few decades in furthering our understanding of the growth of cosmic structure. Nonetheless, there remains a great deal of uncertainty regarding the precise details of the complex baryonic physics that regulate galaxy formation. Any theory of star formation in galaxies must encompass the radiative cooling of gas into dark matter haloes, the formation of a turbulent, multiphase interstellar medium (ISM), the efficiency with which molecular gas is able to collapse into cores and ultimately stars, and the subsequent interaction of those stars with th
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Jose, Jessy, Jinyoung S. Kim, Gregory J. Herczeg, et al. "STAR FORMATION IN W3—AFGL 333: YOUNG STELLAR CONTENT, PROPERTIES, AND ROLES OF EXTERNAL FEEDBACK." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621216.

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One of the key questions in the field of star formation is the role of stellar feedback on the subsequent star formation process. The W3 giant molecular cloud complex at the western border of the W4 super bubble is thought to be influenced by the massive stars in W4. This paper presents a study of the star formation activity within AFGL. 333, a similar to 104 M-circle dot cloud within W3, using deep JHK(s) photometry obtained from the NOAO Extremely Wide Field Infrared Imager combined with Spitzer IRAC and MIPS photometry. Based on the infrared excess, we identify 812 candidate young stellar o
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Lochhaas, Cassandra Derrick. "Stellar Feedback in Galaxies, Its Impact on the Circumgalactic Medium, and the Importance of Radiative Cooling." The Ohio State University, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=osu1562676332648711.

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Grisdale, Kearn. "The role of stellar feedback on the structure of the ISM and star formation in galaxies." Thesis, University of Surrey, 2017. http://epubs.surrey.ac.uk/841384/.

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Stellar feedback refers to the injection of energy, momentum and mass into the interstellar medium (ISM) by massive stars. This feedback owes to a combination of ionising radiation, radiation pressure, stellar winds and supernovae and is likely responsible both for the inefficiency of star formation in galaxies, and the observed super-sonic turbulence of the ISM. In this thesis, I study how stellar feedback shapes the ISM thereby regulating galaxy evolution. In particular, I focus on three key questions: (i) How does stellar feedback shape the gas density distribution of the ISM? (ii) How does
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DECATALDO, DAVIDE. "The Effect of Stellar and Quasar Feedback on the Interstellar Medium: Structure and Lifetime of Molecular Clouds." Doctoral thesis, Scuola Normale Superiore, 2020. http://hdl.handle.net/11384/90712.

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Serrano, Medina Sac Nicte Xiomara [Verfasser]. "Radio emission from massive Young Stellar Objects and their surroundings : Characterization and feedback / Sac Nicte Xiomara Serrano Medina." Bonn : Universitäts- und Landesbibliothek Bonn, 2020. http://d-nb.info/1221668978/34.

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Books on the topic "Stellar feedbacks"

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Emerick, Andrew James. Stellar Feedback and Chemical Evolution In Dwarf Galaxies. [publisher not identified], 2019.

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Hummels, Cameron Bryce. Comparing Simulations and Observations of Galaxy Evolution: Methods for Constraining the Nature of Stellar Feedback. [publisher not identified], 2012.

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DAEC Workshop (3rd 1992 Observatoire de Paris-Meudon). The feedback of chemical evolution on the stellar content of galaxies: Proceedings of the 3rd DAEC Workshop, Observatoire de Paris/Meudon October 12-16, 1992. Imprimerie de l'Observatoire de Paris, Section Meudon, 1992.

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Hoelscher, Jason A. Art as Information Ecology. Duke University Press, 2021. http://dx.doi.org/10.1215/9781478021681.

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In Art as Information Ecology, Jason A. Hoelscher offers not only an information theory of art but an aesthetic theory of information. Applying close readings of the information theories of Claude Shannon and Gilbert Simondon to 1960s American art, Hoelscher proposes that art is information in its aesthetic or indeterminate mode—information oriented less toward answers and resolvability than toward questions, irresolvability, and sustained difference. These irresolvable differences, Hoelscher demonstrates, fuel the richness of aesthetic experience by which viewers glean new information and ins
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Book chapters on the topic "Stellar feedbacks"

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Ristikangas, Vesa, and Tapani Rinne. "Feedback puts wings on development." In Stellar Management Teams. Routledge, 2018. http://dx.doi.org/10.4324/9781351244114-14.

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Letokhov, Vladilen S. "Noncoherent Feedback in Space Masers and Stellar Lasers." In Amazing Light. Springer New York, 1996. http://dx.doi.org/10.1007/978-1-4612-2378-8_41.

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Fender, Rob, and Teo Muñoz-Darias. "The Balance of Power: Accretion and Feedback in Stellar Mass Black Holes." In Astrophysical Black Holes. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-19416-5_3.

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Elgendy, Hoda E., Mashhoor A. Al-Wardat, Hassan B. Haboubi, Lin R. Benchi, Abdallah M. Hussein, and Hussein M. Elmehdi. "A Complete Analysis of Subgiant Stellar Systems III: Hip70868." In Springer Proceedings in Physics. Springer Nature Singapore, 2025. https://doi.org/10.1007/978-981-96-3276-3_21.

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Abstract This study utilizes “Al-Wardat’s method for analysing binary and multiple stellar systems” to estimate a set of parameters for the binary system Hip70868. The method compares the system’s observational magnitudes, color indices, and spectral energy distribution (SED) and synthetic SEDs generated through atmospheric modeling of each component. Feedback-adjusted parameters and an iterative approach were employed to achieve the best fit between observational (including the latest measurements of Gaia, release DR3) and synthetic spectral energy distributions. The findings were completed using the distance of 71.89 pc given by Hipparcos 2007’s new reduction. The individual components’ parameters for the system were derived afterward. The parameters obtained for the individual components are as follows: Component A has an effective temperature (Teff) of 6072 ± 50 K, a surface gravity (log ga) of 4.50 ± 0.05, and a radius (Ra) of 1.40 ± 0.07 $${\text{R}}_{\odot}$$ R ⊙ . Component B has a (Teff) of 5887 ± 50 K, a (log gb) of 4.40 ± 0.05, and a radius (Rb) of 1.326 ± 0.07 $${\text{R}}_{\odot}$$ R ⊙ . The spectral types of the components were found to be F9 IV and G1 IV, respectively. The findings from this analysis were utilized to accurately position the two system components on the Hertzsprung-Russell (H-R) diagram and the evolutionary tracks. The analysis shows that the components have transitioned from the main sequence to the sub-giant stage of their evolution.
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Latniak, Erich, and Jennifer Schäfer. "Operative Führungskräfte in virtuellen Kontexten stärken und gesund erhalten." In Digitale Führung und Zusammenarbeit. Springer Berlin Heidelberg, 2024. http://dx.doi.org/10.1007/978-3-662-63764-7_5.

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ZusammenfassungDer Einsatz moderner Informations- und Kommunikationstechnologien (IKT) bringt spezifische Anforderungen, Bedingungen und Auswirkungen für die Beschäftigten mit sich. Während für die Beschäftigten hierzu Forschungsergebnisse vorliegen, fehlen diese insbesondere für die operativen Führungskräfte in virtuellen Teams weitgehend, sodass es auch schwierig ist, Empfehlungen für die Gestaltung der Arbeit und Unterstützung der operativen Führungskräfte virtueller Teams zu geben. In diesem Beitrag wird daher die Ressourcen- und Belastungssituation operativer Führungskräfte in virtuellen Teams analysiert und Ansätze zu deren Unterstützung vorgestellt, um diese in virtuellen Kontexten zu stärken und gesund zu erhalten. Dazu erläutern wir zunächst den konzeptionellen Hintergrund unseres Vorgehens und das dafür entwickelte Feedback- und Reflexionstool. Anschließend stellen wir die explorativen Befunde zur Ressourcen- und Belastungssituation der teilnehmenden operativen Führungskräfte in virtuellen Arbeitskontexten sowie die daraus abgeleiteten Handlungsempfehlungen zur Gestaltung und Regulierung der Arbeitssituation vor, die zu einem verbesserten Ressourcenmanagement der operativen Führungskräfte beitragen sollen. Zur Abschätzung des Nutzens der eingesetzten Instrumente sowie der möglichen Wirkungen der Empfehlungen aus den Feedbackgesprächen haben eine Nachbefragung der teilnehmenden operativen Führungskräfte durchgeführt, deren Ergebnisse und weitere Hinweise zur Nutzung und Anwendung des entwickelten Feedback- und Reflexionstools abschließend dargestellt werden.
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Antoni, Conny H., and A. T. Niesen. "vLead-OrgaCheck – Identifikation von Stellschrauben zur Verbesserung der digitalen Zusammenarbeit." In Digitale Führung und Zusammenarbeit. Springer Berlin Heidelberg, 2024. http://dx.doi.org/10.1007/978-3-662-63764-7_2.

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ZusammenfassungOb ein Unternehmen gut für die digitale Zusammenarbeit aufgestellt ist, hängt vom Zusammenspiel unterschiedlicher Faktoren ab. In diesem Beitrag wird das Online-Befragungs- und Feedback-Instrument OrgaCheck vorgestellt (orgacheck.vlead.de), das wir in Kooperation mit einem Unternehmen aus dem IT-Bereich entwickelt haben und das die relevantesten Faktoren für eine erfolgreiche Digitalisierung auf den Ebenen Technik, Organisation und Personal und deren Auswirkungen auf die digitale Zusammenarbeit aus Sicht von Führungskräften und Mitarbeitenden erfasst. Unternehmen können individuelle Schwerpunkte in der Befragung setzen, indem sie Aspekte aus- oder abwählen. Die Befragungsergebnisse werden durch das Tool automatisiert ausgewertet und in Berichten für das Gesamtunternehmen und für einzelne Abteilungen automatisiert zusammengefasst. Die Unternehmen erhalten zusammen mit dem Feedback zugleich Handlungshinweise für die jeweiligen Faktoren mit auffälligen Ergebnissen und können dadurch an den für sie entscheidenden Stellschrauben drehen. In dem Beitrag erläutern wir zunächst unsere theoretischen Überlegungen, die dem OrgCheck zugrunde liegen, stellen unsere eigenen Studienergebnisse vor und beschreiben dann im Detail das Instrument und seine Funktionalitäten. Im Anschluss werden erste Evaluationsergebnisse aus vier Unternehmen zu den Einsatzmöglichkeiten vorgestellt, die den Mehrwert des Umfragetools aufzeigen. Der Beitrag schließt mit einem Ausblick auf die Einsatzmöglichkeiten und den Nutzen des OrgaChecks insbesondere für kleine und mittlere Unternehmen.
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Bastian, Morten, and Andreas Mühling. "Erste Schritte zur automatisierten Generation von Items in einem webbasierten Tracingsystem." In Die Zukunft des MINT-Lernens – Band 1. Springer Berlin Heidelberg, 2022. http://dx.doi.org/10.1007/978-3-662-66131-4_12.

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ZusammenfassungDer Beitrag stellt die Ergebnisse einer Vorstudie und einer experimentellen Studie (N = 273) in der Sekundarstufe und der Universität im Kontext der Programmierung, genauer der Programmablaufverfolgung (Tracing), vor. Das Ziel ist die automatische Generierung von Items in einem adaptiven Testsystem, die bekannte Fehlvorstellungen sichtbar machen können. Verglichen werden dazu zunächst die empirisch unter Lernenden ermittelten Schwierigkeiten bekannter Items mit den Schwierigkeiten, die aus einem theoretischen Vorhersagemodell abgeleitet werden, sowie mit einem Rating von Experten. Darauf aufbauend werden Items anhand von einfachen Regeln generiert und in einer Hauptstudie deren durch die Regeln vorhergesagte Schwierigkeitsrangfolge empirisch überprüft. Die Ergebnisse zeigen, dass eine solche regelbasierte Generierung von Items vielversprechend ist. Bestimmte Programmkonstrukte sind hinsichtlich ihrer Schwierigkeit auf diese Weise gut klassifizierbar und können so für die automatisierte Itemkonstruktion genutzt werden. Praktisch erlauben solche adaptiven Testverfahren in kurzer Zeit die Diagnose von Fehlvorstellungen, die eine große Hürde in der Programmierausbildung darstellen. Aufgrund der Regeln und des Itemformats ist es darüber hinaus möglich, gezielt Feedback zu den Fehlvorstellungen an die Testerinnen und Tester, oder auch die Lernenden selbst, zu geben.
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"Stellar Feedback." In Star Formation. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813142046_0008.

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Loeb, Abraham, and Steven R. Furlanetto. "Stellar Feedback and Galaxy Formation." In The First Galaxies in the Universe. Princeton University Press, 2013. http://dx.doi.org/10.23943/princeton/9780691144917.003.0006.

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This chapter studies radiative, mechanical, and chemical feedback in the earliest gaseous clouds, taking up the thread of discussion in the previous chapter to consider the influences placed on the formation of second-generation stars. While the feedback effects are sufficiently complex that a complete description of them is well beyond the capabilities of present-day computer simulations, the general principles that underlie them are well known. Therefore, the chapter focuses on these principles and then briefly sketches the global picture. Feedback is important in all galaxies, and many of the principles that are discussed in this chapter apply on a much wider scale than just the first stars and galaxies.
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"Chapter Six. Stellar Feedback and Galaxy Formation." In The First Galaxies in the Universe. Princeton University Press, 2013. http://dx.doi.org/10.1515/9781400845606.174.

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Conference papers on the topic "Stellar feedbacks"

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Padilla, Nelson D., Claudia Lagos, Michael Strauss, Sebastian Heinz, and Eric Wilcots. "Stellar Disc—Active Nucleus Alignments in the SDSS." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293009.

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Hueckstaedt, Robert, Daniel Whalen, Thomas McConkie, Daniel J. Whalen, Volker Bromm, and Naoki Yoshida. "Local Radiative Feedback: The Rise of Early Stellar Populations." In THE FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE. AIP, 2010. http://dx.doi.org/10.1063/1.3518869.

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Kubátová, Brankica, and Dorottya Szécsi. "SPECTRAL CHARACTERISTICS OF FAST ROTATING METAL-POOR MASSIVE STARS." In XX Serbian Astronomical Conference. Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia, 2024. https://doi.org/10.69646/aob104p099.

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Abstract. Low-metallicity massive stars are assumed to be progenitors of certain supernovae, gamma-ray bursts, and gravitational wave emitting mergers. These exotic phenomena contribute to their host galaxies through strong ionizing radiation and mechanical feedback. Here we investigate a certain type of very metal-poor (0.02 xxx Z xxx 0) hot massive single stars that rotate fast and evolve chemically homogeneously. Combining state-of-the-art theories of stellar evolution and stellar atmospheres modelling we predict synthetic spectra of these stars corresponding to different masses and evoluti
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CIARDI, B., and A. FERRARA. "FIR/SUB-MM LINE EMISSION FROM THE FIRST OBJECTS: TESTING THE STELLAR FEEDBACK." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0029.

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Bowen, Maitland, Brian T. Fleming, Briana L. Indahl, et al. "Preflight characterization of the SPRITE CubeSat: a far-UV imaging spectrograph for stellar feedback in local galaxies." In Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, edited by Jan-Willem A. den Herder, Kazuhiro Nakazawa, and Shouleh Nikzad. SPIE, 2024. http://dx.doi.org/10.1117/12.3020453.

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Indahl, Briana, Brian Fleming, Dmitry Vorobiev, et al. "Status and mission operations of the SPRITE 12U CubeSat: a probe of star formation feedback from stellar to galactic scales with far-UV imaging spectroscopy." In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXIII, edited by Oswald H. Siegmund and Keri Hoadley. SPIE, 2023. http://dx.doi.org/10.1117/12.2677737.

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Reports on the topic "Stellar feedbacks"

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Li, Richard. LegalOne Stellar Accolade 2023 - China. LegalOne Global Limited, 2023. http://dx.doi.org/10.62436/a-1702224947429.

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Abstract:
The LegalOne Stellar Accolade is an honour roll serving as an illustrious recognition of the practical prowess and expertise of legal professionals. The evaluation process is rooted in the thorough assessment of commercial projects submitted by the legal professionals. LegalOne’s editorial team reviews each submission, encompassing a broad spectrum of commercial transactions, dispute cases, and intellectual property matters. The declaration of the LegalOne Stellar Accolade winners is based on a composite of factors, include the quality and level of LegalOne Merits ratings awarded to the applic
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Dudenbostel, Tobias, and David Heckenberg. Bedarfsanalyse Qualifizierungsoffensive. Endbericht an das Bundesministerium für Digitalisierung und Wirtschaftsstandort (BMDW). BMDW - Bundesministerium für Digitalisierung und Wirtschaftsstandort, 2022. http://dx.doi.org/10.22163/fteval.2022.564.

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Seit 2011 unterstützt das Bundesministerium für Digitalisierung und Wirtschaftsstandort (BMDW) mit dem Programm Qualifizierungsoffensive bzw. Forschungskompetenzen für die Wirtschaft den systematischen Auf- und Ausbau von Kompetenzen von Unternehmen und ihrer Mitarbeiter*innen in den Bereichen Forschung, Technologie, Entwicklung, Innovation und Digitalisierung. Das Programm wird von der FFG administriert und umfasst heute Konsortialprojekte zwischen Wissenschaft und Wirtschaft von verschiedener Länge und Intensität (Innovationscamp S, M, und Digital Pro Bootcamp) sowie den Digital Skills Schec
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