Academic literature on the topic 'Star-forming'

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Star-forming.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Star-forming"

1

Kaifu, Norio. "Star forming regions." Vistas in Astronomy 31 (1988): 199–206. http://dx.doi.org/10.1016/0083-6656(88)90202-4.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Ivison, R. J., J. Richard, A. D. Biggs, et al. "Giant star-forming clumps?" Monthly Notices of the Royal Astronomical Society: Letters 495, no. 1 (2020): L1—L6. http://dx.doi.org/10.1093/mnrasl/slaa046.

Full text
Abstract:
ABSTRACT With the spatial resolution of the Atacama Large Millimetre Array (ALMA), dusty galaxies in the distant Universe typically appear as single, compact blobs of dust emission, with a median half-light radius, ≈1 kpc. Occasionally, strong gravitational lensing by foreground galaxies or galaxy clusters has probed spatial scales 1–2 orders of magnitude smaller, often revealing late-stage mergers, sometimes with tantalizing hints of sub-structure. One lensed galaxy in particular, the Cosmic Eyelash at z = 2.3, has been cited extensively as an example of where the interstellar medium exhibits
APA, Harvard, Vancouver, ISO, and other styles
3

Myers, Philip C. "Star-forming Filament Models." Astrophysical Journal 838, no. 1 (2017): 10. http://dx.doi.org/10.3847/1538-4357/aa5fa8.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Álvarez-Álvarez, Mar, Ángeles I. Díaz, and Marcelo Castellanos. "Massive star population in circumnuclear star-forming regions." Symposium - International Astronomical Union 212 (2003): 537–38. http://dx.doi.org/10.1017/s0074180900212746.

Full text
Abstract:
Due to their high luminosity, the importance of understanding the massive star formation and evolution of giant Hii regions has become more and more evident in the last few years. A mayor scenario where giant H ii regions form and develop are the very inner parts of some galaxies. These bursts frequently are arranged in a ring-like pattern. We present a study of the stellar populations and gas physical conditions in circumnuclear star-forming regions (CNSFR) based on broad- and narrow-band photometry and spectrophotometric data, which have been analyzed with the use of evolutionary population
APA, Harvard, Vancouver, ISO, and other styles
5

Kaltcheva, Nadia, Vincent Fabbri, Timothy Conard, and Valeri Golev. "Cepheus Star-Forming Field Revisited." International Journal of Astronomy and Astrophysics 03, no. 04 (2013): 472–79. http://dx.doi.org/10.4236/ijaa.2013.34054.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Barthel, Peter. "Star-forming AGN host galaxies." New Astronomy Reviews 45, no. 9-10 (2001): 591–99. http://dx.doi.org/10.1016/s1387-6473(01)00139-7.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Nisini, Brunella, and Teresa Giannini. "H2O in Star Forming Regions." Highlights of Astronomy 12 (2002): 67–69. http://dx.doi.org/10.1017/s1539299600012855.

Full text
Abstract:
AbstractThis paper will review the importance of the water molecule in the various stages of the star formation process, addressing in particular how the recent observations obtained with the ISO and SWAS satellites have challenged the existing theoretical models.
APA, Harvard, Vancouver, ISO, and other styles
8

Bartkiewicz, Anna, and Huib Jan van Langevelde. "Masers in star forming regions." Proceedings of the International Astronomical Union 8, S287 (2012): 117–26. http://dx.doi.org/10.1017/s1743921312006771.

Full text
Abstract:
AbstractMaser emission plays an important role as a tool in star formation studies. It is widely used for deriving kinematics, as well as the physical conditions of different structures, hidden in the dense environment very close to the young stars, for example associated with the onset of jets and outflows. We will summarize here the recent observational and theoretical progress on this topic since the last maser symposium: the IAU Symposium 242 in Alice Springs.
APA, Harvard, Vancouver, ISO, and other styles
9

Hodapp, Klaus-Werner, and John Rayner. "The S106 star-forming region." Astronomical Journal 102 (September 1991): 1108. http://dx.doi.org/10.1086/115937.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Barthel, P. D. "Star-forming QSO host galaxies." Astronomy & Astrophysics 458, no. 1 (2006): 107–11. http://dx.doi.org/10.1051/0004-6361:20053591.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Star-forming"

1

Lee, Pawel. "Structure in star forming regions." Thesis, University of Sheffield, 2016. http://etheses.whiterose.ac.uk/12395/.

Full text
Abstract:
Stars form in clumpy, highly substructured environments. In this thesis I set up N-body simulations of substructured star forming regions and investigate the impact that the substructure has on the survival of the star forming regions. I also present a broad range of methods used in other fields to quantify and identify structure. I discuss their strengths and shortcomings and assess their suitability for use in astronomical contexts. I use the Q and Λ methods to compare the distributions of class I and class II sources in observed star forming regions to learn more about the dynamical evoluti
APA, Harvard, Vancouver, ISO, and other styles
2

Gledhill, Timothy Michael. "Optical polarimetry of star forming regions." Thesis, Durham University, 1987. http://etheses.dur.ac.uk/6757/.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Holdship, J. R. "Shock chemistry in star forming environments." Thesis, University College London (University of London), 2017. http://discovery.ucl.ac.uk/10027644/.

Full text
Abstract:
Molecules are abundant in many astrophysical environments. The observation of these molecules and the modelling of the chemistry that leads to their formation is a powerful tool for improving our understanding of the regions in which they are found. In this thesis, a chemical model is developed and applied to astrophysical shocks to understand a number of processes in star forming regions. Shocks often result in discontinuous changes in the temperature and density of the gases they affect. The turbulent fragmentation theory of star formation suggests that such shocks are responsible for the ov
APA, Harvard, Vancouver, ISO, and other styles
4

Lacki, Brian Cameron. "Cosmic Rays in Star-Forming Galaxies." The Ohio State University, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=osu1313437011.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Kalari, Venu Madhav. "Disc-accretion in star-forming regions." Thesis, Queen's University Belfast, 2015. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.695381.

Full text
Abstract:
In this thesis, I present new ultraviolet/optical/infrared photometric and spectroscopic observations of pre-main sequence stars (PMS) that have formed either in metal-poor conditions, or in the vicinity of strong ionising radiation. This includes observations of 235 Classical T Tauri stars in the Lagoon Nebula; 63 Classical T Tauril Herbig Ae stars in the Carina Nebula open cluster Trumpler 14; 24 intermediate mass T Tauri stars in the low-Z Sh 2-284 star-forming region; and one Herbig 8[e] PMS candidate in the metal-poor 30 Doradus region. I measure the accretion rates of these PMS stars usi
APA, Harvard, Vancouver, ISO, and other styles
6

Contreras, Peña Carlos Eduardo. "Exteme variables in star forming regions." Thesis, University of Hertfordshire, 2015. http://hdl.handle.net/2299/15590.

Full text
Abstract:
The notion that low- to intermediate-mass young stellar objects (YSOs) gain mass at a constant rate during the early stages of their evolution appears to be challenged by observations of YSOs suffering sudden increases of the rate at which they gain mass from their circumstellar discs. Also, this idea that stars spend most of their lifetime with a low accretion rate and gain most of their final mass during short-lived episodes of high accretion bursts, helps to solve some long-standing problems in stellar evolution. The original classification of eruptive variables divides them in two separate
APA, Harvard, Vancouver, ISO, and other styles
7

Mineo, Stefano. "X-ray emission from star-forming galaxies." Diss., lmu, 2011. http://nbn-resolving.de/urn:nbn:de:bvb:19-134839.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Maskoliūnas, Marius. "Investigation of star forming regions in Cepheus." Doctoral thesis, Lithuanian Academic Libraries Network (LABT), 2014. http://vddb.library.lt/obj/LT-eLABa-0001:E.02~2014~D_20140203_133341-51153.

Full text
Abstract:
The interstellar matter in the Galaxy is concentrated in a thin layer close to the galactic plane, mostly in spiral arms. Most of the interstellar matter is in a form of atomic and molecular gas and only 1% of its mass is in a form of small (0.01 – 0.1 µm) dust grains which absorb and scatter the light of stars and cause the interstellar extinction. A part of interstellar gas and dust are in a diffuse form and fill the space with density which exponentially decreases with the distance from the galactic plane. However, in the spiral arms gigantic molecular clouds are present which play an out
APA, Harvard, Vancouver, ISO, and other styles
9

Juárez, Rodríguez Carmen. "Collapse scenarios in magnetized star-forming regions." Doctoral thesis, Universitat de Barcelona, 2017. http://hdl.handle.net/10803/459253.

Full text
Abstract:
Turbulence, magnetic fields and gravity driven flows are important for the formation of new stars. Although magnetic fields have been proven to be important in the formation of stars, only a few works have been done combining magnetic field and kinematic information. Such studies are important to analyze both gravity and gas dynamics and be able to compare them with the magnetic field. In this thesis we will combine dust polarization studies with kinematic analysis towards different star-forming regions. We aim to study the physical properties at core scales (<0.1 pc) from molecular line and
APA, Harvard, Vancouver, ISO, and other styles
10

Simon, Robert. "Multiline CN observations of star forming regions." [S.l. : s.n.], 1997. http://deposit.ddb.de/cgi-bin/dokserv?idn=955972264.

Full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "Star-forming"

1

Peimbert, Manuel, and Jun Jugaku, eds. Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Torres, Diego F., and Olaf Reimer, eds. Cosmic Rays in Star-Forming Environments. Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-35410-6.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

D, Kunth, Trinh Xuan Thuan, and Tran J. Thanh Van, eds. Star-forming dwarf galaxies and related objects. Frontieres, 1985.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
4

Cowley, William. The Nature of Dusty Star-Forming Galaxies. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-66748-5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

HARTQUIST, T. W., J. M. PITTARD, and S. A. E. G. FALLE, eds. Diffuse Matter from Star Forming Regions to Active Galaxies. Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-5425-9.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Olofsson, Kjell. Spectral evolutionary synthesis models of metal-poor star forming regions. Uppsala Astronomical Observatory, 1988.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
7

Workshop on Star-Forming Dwarf Galaxies and Related Objects (1985 Institut d'Astrophysique, Paris). Proceedings of the Workshop on Star-Forming Dwarf Galaxies and related objects, July 1-3, 1985, Institut d'Astrophysique, Paris, France. Editions Frontieres, 1986.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
8

1941-, Peimbert Manuel, and Jugaku Jun 1927-, eds. Star forming regions: Proceedings of the 115th Symposium of the International Astronomical Union held in Tokyo, Japan, November 11-15, 1985. D. Reidel Pub. Co., 1987.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
9

Strickland, David Kendal. X-ray emission from starburst-driven galactic winds: A confrontation between the theory and observations of the violent interstellar medium in star forming galaxies. University of Birmingham, 1998.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
10

Bo, Reipurth, and Astronomical Society of the Pacific., eds. Handbook of star forming regions. Astronomical Society of the Pacific, 2008.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Book chapters on the topic "Star-forming"

1

Schulz, Norbert S. "Star-Forming Regions." In The Formation and Early Evolution of Stars. Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-23926-7_11.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Wilking, B. A., L. G. Mundy, and R. D. Schwartz. "The Circumstellar Environment of LkHα 234." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_115.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Di Fazio, A. "A New Theory of Star Formation: Analytical Mass Function and Star Formation Rate." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_143.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Shuter, W. L. H., R. L. Dickman, and C. Klatt. "21 cm Line Study of Large Scale Density Fluctuations in the Taurus Molecular Complex." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_15.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Tomisaka, Kohji. "Formation of Giant Molecular Clouds by Coagulation of Small Molecular Clouds in a Spiral Gravitational Potential." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_160.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Wynn-Williams, C. G. "Bursts of Star Formation in Galaxies." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_172.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

García-Barreto, J. A., and P. Pişmiş. "Radio Continuum Observations of the Barred Galaxy NGC 4314." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_183.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Rengarajan, T. N., and R. P. Verma. "FIR and Blue Luminosities and Gas Mass in Spiral Galaxies." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_203.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Saito, Shuji. "Laboratory Microwave Spectroscopy of Interstellar Molecules." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_33.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Tomita, Yoshio. "Observation of the Large Scale Structures of Dark Clouds." In Star Forming Regions. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4782-5_6.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Star-forming"

1

Charnley, S. B. "Chemistry of star-forming cores." In The 50th international meeting of physical chemistry: Molecules and grains in space. AIP, 1994. http://dx.doi.org/10.1063/1.46622.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Kelm, Birgit. "Single Star-Forming Galaxies and Star-Forming Galaxies in SF + SF and Mixed Pairs." In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2034966.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Lisitsin, D. D., and A. V. Kuzin. "Identification of extragalactic star forming complexes." In Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой «Астрономия и исследование космического пространства». Ural University Press, 2021. http://dx.doi.org/10.15826/b978-5-7996-3229-8.08.

Full text
Abstract:
We developed a technique for selecting star forming complexes in external galaxies based on an analysis of radiation maps in various spectral bands. Using this method, we identified star formation complex candidates in 17 nearby galaxies applying three criteria. These criteria are polycyclic aromatic hydrocarbon emission, dust emission, and ultraviolet young star emission. Relating the information derived from these criteria, we made a sample of star forming regions suitable for revealing correlations between various star formation tracers.
APA, Harvard, Vancouver, ISO, and other styles
4

Porter, Troy. "Cosmic rays in star-forming galaxies." In CENTENARY SYMPOSIUM 2012: DISCOVERY OF COSMIC RAYS. AIP, 2013. http://dx.doi.org/10.1063/1.4792557.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Padoan, P., A. G. Kritsuk, T. Lunttila, et al. "MHD Turbulence In Star-Forming Clouds." In PLASMAS IN THE LABORATORY AND THE UNIVERSE: Interactions, Patterns, and Turbulence. AIP, 2010. http://dx.doi.org/10.1063/1.3460128.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Gerssen, Joris, David Wilman, Lise Christensen, Victor P. Debattista, and C. C. Popescu. "Mapping Star Forming & AGN Galaxies." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458498.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Pierrick, Martin. "Cosmic Rays in star forming galaxies." In Cosmic Rays and the InterStellar Medium. Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.221.0018.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Romero, Gustavo E., Felix A. Aharonian, Werner Hofmann, and Frank Rieger. "Gamma rays from star-forming regions." In HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP, 2008. http://dx.doi.org/10.1063/1.3076825.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Caillault, Jean-Pierre. "Stellar clusters and star-forming regions." In The soft x-ray cosmos: ROSAT science symposium and data analysis workshop. AIP, 1994. http://dx.doi.org/10.1063/1.46667.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Wiebe, Dmitry. "Dust in Star Forming Regions - A Review." In Frontier Research in Astrophysics – II. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.269.0023.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Reports on the topic "Star-forming"

1

O'Shea, Brian. Forming a Primordial Star in a Relic HII Region. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/839853.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Hidetoshi, Sano. Star Forming Dense Cloud Cores in the TeV -ray SNR RX J1713.7-3946. Office of Scientific and Technical Information (OSTI), 2010. http://dx.doi.org/10.2172/993416.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Riveros, Guillermo, Felipe Acosta, Reena Patel, and Wayne Hodo. Computational mechanics of the paddlefish rostrum. Engineer Research and Development Center (U.S.), 2021. http://dx.doi.org/10.21079/11681/41860.

Full text
Abstract:
Purpose – The rostrum of a paddlefish provides hydrodynamic stability during feeding process in addition to detect the food using receptors that are randomly distributed in the rostrum. The exterior tissue of the rostrum covers the cartilage that surrounds the bones forming interlocking star shaped bones. Design/methodology/approach – The aim of this work is to assess the mechanical behavior of four finite element models varying the type of formulation as follows: linear-reduced integration, linear-full integration, quadratic-reduced integration and quadratic-full integration. Also presented i
APA, Harvard, Vancouver, ISO, and other styles
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!