Relevant bibliographies by topics / Low mass stars. Dwarf stars

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

Academic literature on the topic 'Low mass stars. Dwarf stars'

Author: Grafiati
Published: 4 June 2021
Last updated: 15 February 2022

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Journal articles on the topic "Low mass stars. Dwarf stars"

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Kepler, S. O., Alejandra Daniela Romero, Ingrid Pelisoli, and Gustavo Ourique. "White Dwarf Stars." International Journal of Modern Physics: Conference Series 45 (January 2017): 1760023. http://dx.doi.org/10.1142/s2010194517600230.

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White dwarf stars are the final stage of most stars, born single or in multiple systems. We discuss the identification, magnetic fields, and mass distribution for white dwarfs detected from spectra obtained by the Sloan Digital Sky Survey up to Data Release 13 in 2016, which lead to the increase in the number of spectroscopically identified white dwarf stars from 5[Formula: see text]000 to 39[Formula: see text]000. This number includes only white dwarf stars with [Formula: see text], i.e., excluding the Extremely Low Mass white dwarfs, which are necessarily the byproduct of stellar interaction
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France, Kevin, R. O. Parke Loyd, and Alex Brown. "Ultraviolet and X-ray irradiance and flares from low-mass exoplanet host stars." Proceedings of the International Astronomical Union 11, S320 (2015): 370–75. http://dx.doi.org/10.1017/s1743921315010765.

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AbstractThe spectral and temporal behavior of exoplanet host stars is a critical input to models of the chemistry and evolution of planetary atmospheres. High-energy photons (X-ray to NUV) from these stars regulate the atmospheric temperature profiles and photochemistry on orbiting planets, influencing the production of potential “biomarker” gases. We report first results from the MUSCLES Treasury Survey, a study of time-resolved UV and X-ray spectroscopy of nearby M and K dwarf exoplanet host stars. This program uses contemporaneous Hubble Space Telescope and Chandra (or XMM) observations to
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Kepler, S. O., Ingrid Pelisoli, Detlev Koester, et al. "White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14." Monthly Notices of the Royal Astronomical Society 486, no. 2 (2019): 2169–83. http://dx.doi.org/10.1093/mnras/stz960.

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ABSTRACT White dwarfs carry information on the structure and evolution of the Galaxy, especially through their luminosity function and initial-to-final mass relation. Very cool white dwarfs provide insight into the early ages of each population. Examining the spectra of all stars with 3σ proper motion in the Sloan Digital Sky Survey Data Release 14, we report the classification for 20 088 spectroscopically confirmed white dwarfs, plus 415 hot subdwarfs, and 311 cataclysmic variables. We obtain Teff, log g, and mass for hydrogen atmosphere white dwarf stars (DAs), warm helium atmosphere white d
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Jones, Hugh R. A., Yakiv Pavlenko, Serena Viti, et al. "Carbon monoxide in low-mass dwarf stars." Monthly Notices of the Royal Astronomical Society 358, no. 1 (2005): 105–12. http://dx.doi.org/10.1111/j.1365-2966.2005.08736.x.

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Giampapa, M. S., R. Rosner, V. Kashyap, T. A. Fleming, J. H. M. M. Schmitt, and J. A. Bookbinder. "The Coronae of Low-Mass Dwarf Stars." Astrophysical Journal 463 (June 1996): 707. http://dx.doi.org/10.1086/177284.

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Ruiz, María Teresa. "Do Low Luminosity Stars Matter?" Proceedings of the International Astronomical Union 5, H15 (2009): 47–60. http://dx.doi.org/10.1017/s1743921310008185.

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AbstractHistorically, low luminosity stars have attracted very little attention, in part because they are difficult to see except with large telescopes, however, by neglecting to study them we are leaving out the vast majority of stars in the Universe. Low mass stars evolve very slowly, it takes them trillions of years to burn their hydrogen, after which, they just turn into a He white dwarf, without ever going through the red giant phase. This lack of observable evolution partly explains the lack of interest in them. The search for the “missing mass” in the galactic plane turned things around
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Jones, Hugh R. A., John Barnes, Mikko Tuomi, James S. Jenkins, and Guillem Anglada-Escude. "Radial velocity studies of cool stars." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 372, no. 2014 (2014): 20130088. http://dx.doi.org/10.1098/rsta.2013.0088.

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Our current view of exoplanets is one derived primarily from solar-like stars with a strong focus on understanding our Solar System. Our knowledge about the properties of exoplanets around the dominant stellar population by number, the so-called low-mass stars or M dwarfs, is much more cursory. Based on radial velocity discoveries, we find that the semi-major axis distribution of M dwarf planets appears to be broadly similar to those around more massive stars and thus formation and migration processes might be similar to heavier stars. However, we find that the mass of M dwarf planets is relat
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Rana, N. C. "Scaleheights of Low Mass Stars from the Luminosity Function of the Local White Dwarfs." International Astronomical Union Colloquium 114 (1989): 152–55. http://dx.doi.org/10.1017/s0252921100099486.

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It is shown that a combination of the observed luminosity function of the local white dwarfs and the theoretical cooling rates of a typical white dwarf suggests an approximately constant rate of formation of the white dwarfs. This rate is found to be about a factor of three lower than the observed birthrate of their immediate progenitors. This discrepancy is here interpreted as a three-fold increase in the scaleheight of the white dwarfs due to dynamical interaction with stars, molecular clouds; an average white dwarf being much more aged than an average progenitor. Since the low mass stars on
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Sánchez Arias, Julieta P., Alejandra D. Romero, Alejandro H. Córsico та ін. "Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and δ Scuti stars". Astronomy & Astrophysics 616 (серпень 2018): A80. http://dx.doi.org/10.1051/0004-6361/201731808.

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Context. Pulsating extremely low-mass pre-white dwarf stars (pre-ELMV), with masses between ~0.15 M⊙ and ~0.30 M⊙, constitute a new class of variable stars showing g- and possibly p-mode pulsations with periods between 320 and 6000 s (frequencies between 14.4 and 270 c/d), driven by the κ mechanism operating in the second He ionization zone. On the other hand, main sequence δ Scuti stars, with masses between 1.2 and 2.5 M⊙, pulsate in low-order g and p modes with periods in the range [700–28 800] s (frequencies in the range [3–123] c/d), driven by the κ mechanism operating in the He II ionizat
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Stamatellos, Dimitris, and Anthony Whitworth. "The formation of brown dwarfs in discs: Physics, numerics, and observations." Proceedings of the International Astronomical Union 6, S270 (2010): 223–26. http://dx.doi.org/10.1017/s174392131100041x.

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AbstractA large fraction of brown dwarfs and low-mass stars may form by gravitational fragmentation of relatively massive (a few 0.1 M⊙) and extended (a few hundred AU) discs around Sun-like stars. We present an ensemble of radiative hydrodynamic simulations that examine the conditions for disc fragmentation. We demonstrate that this model can explain the low-mass IMF, the brown dwarf desert, and the binary properties of low-mass stars and brown dwarfs. Observing discs that are undergoing fragmentation is possible but very improbable, as the process of disc fragmentation is short lived (discs
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Dissertations / Theses on the topic "Low mass stars. Dwarf stars"

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Krawchuk, Curtis A. P. "The determination of metallicity and temperature of low-mass stars using broad-band photometry." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1997. http://www.collectionscanada.ca/obj/s4/f2/dsk2/tape15/PQDD_0035/MQ27361.pdf.

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Riaz, Basmah. "A study of circumstellar disk properties in low-mass stars and brown dwarfs." Access to citation, abstract and download form provided by ProQuest Information and Learning Company; downloadable PDF file, 129 p, 2008. http://proquest.umi.com/pqdweb?did=1597616011&sid=8&Fmt=2&clientId=8331&RQT=309&VName=PQD.

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Marks, M., E. L. Martín, V. J. S. Béjar, et al. "Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/625997.

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Context. One of the key questions of the star formation problem is whether brown dwarfs (BDs) form in the manner of stars directly from the gravitational collapse of a molecular cloud core (star-like) or whether BDs and some very low-mass stars (VLMSs) constitute a separate population that forms alongside stars comparable to the population of planets, for example through circumstellar disk (peripheral) fragmentation. Aims. For young stars in Taurus-Auriga the binary fraction has been shown to be large with little dependence on primary mass above approximate to 0.2 M-circle dot, while for BDs t
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Cardoso, Catia Vanessa Varejao. "Observational properties of brown dwarfs : the low-mass end of the mass function." Thesis, University of Exeter, 2012. http://hdl.handle.net/10036/3592.

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Brown dwarfs are objects with sub-stellar masses that are unable to sustain hydrogen burning, cooling down through out their lifetimes. This thesis presents two projects, the study of the IMF of the double cluster, h & χ Persei, and the determination of the dynamical masses of the brown dwarf binary, ε Indi Ba, Bb. The study of a cluster’s population distribution gives us the opportunity to study a statistically meaningful population of objects over a wide range of masses (from massive stars to brown dwarfs), with a similar age and chemical composition providing formation and dynamical evoluti
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Henry, Todd Jackson. "A systematic search for low-mass companions orbiting nearby stars and the calibration of the end of the stellar main sequence." Diss., The University of Arizona, 1991. http://hdl.handle.net/10150/185689.

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We have completed a search for low luminosity companions, including high mass brown dwarfs, to all M dwarfs known within eight parsecs of the sun, and north of -25°. We found six new companions orbiting the survey stars. The masses of the six new secondaries fall between 0.39 and 0.05 M(⊙). Three of the new companions, G208-44B, GL 623B and LHS 1047B, and one previously known secondary in the survey, Ross 614B, are brown dwarf candidates with masses ∼80 Jupiters (0.08 M(⊙)), the dividing line between stars and brown dwarfs. In addition, we provide infrared photometry at J, H and K for all 99 s
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Lew, Ben W. P., Daniel Apai, Yifan Zhou, et al. "CLOUD ATLAS: DISCOVERY OF PATCHY CLOUDS AND HIGH-AMPLITUDE ROTATIONAL MODULATIONS IN A YOUNG, EXTREMELY RED L-TYPE BROWN DWARF." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622769.

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Condensate clouds fundamentally impact the atmospheric structure and spectra of exoplanets and brown dwarfs, but the connections between surface gravity, cloud structure, dust in the upper atmosphere, and the red colors of some brown dwarfs remain poorly understood. Rotational modulations enable the study of different clouds in the same atmosphere, thereby providing a method to isolate the effects of clouds. Here, we present the discovery of high peak-to-peak amplitude (8%) rotational modulations in a low-gravity, extremely red (J-K-s = 2.55) L6 dwarf WISEP J004701.06+680352.1 (W0047). Using t
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Souto, D., K. Cunha, D. A. Garcia-Hernandez, et al. "Chemical Abundances of M-Dwarfs from the Apogee Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624381.

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We report the first detailed chemical abundance analysis of the exoplanet-hosting M-dwarf stars Kepler-138 and Kepler-186 from the analysis of high-resolution (R similar to 22,500) H-band spectra from the SDSS-IV-APOGEE survey. Chemical abundances of 13 elements-C, O, Na, Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, and Fe-are extracted from the APOGEE spectra of these early M-dwarfs via spectrum syntheses computed with an improved line list that takes into account H2O and FeH lines. This paper demonstrates that APOGEE spectra can be analyzed to determine detailed chemical compositions of M-dwarfs. Both
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Kenyon, Michael John. "Low mass stars and brown dwarfs around σ Orionis." Thesis, Keele University, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.409546.

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Cossburn, Martin R. "The study of low-mass stars and brown dwarfs." Thesis, University of Leicester, 1999. http://hdl.handle.net/2381/30616.

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This thesis describes the search for brown dwarfs in open clusters using optical and infrared photometry, optical spectroscopy and surveys using the Hubble Space Telescope (HST). It also includes an observational study of very low-mass stars (VLMS) using a filter combination (I and Z), unused previously in this field enabling the calibration of the colour (I--Z), for future survey work. Following a short introduction explaining the reasons for studying brown dwarfs this thesis reviews the theory of their formation and evolution and describes recent searches for brown dwarfs and their results.
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Pinfield, David J. "Low mass stars and brown dwarfs in open clusters." Thesis, University of Leicester, 1998. http://hdl.handle.net/2381/30612.

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This thesis describes several open cluster searches for very low mass stars (VLM) and brown dwarfs (BD) (M/M? < 0.08). With recent developments in charged coupled devices, it has become possible to survey open clusters to well into the BD regime. The principal aim of this work is to employ these new instruments to conduct such open cluster surveys, to investigate the properties of VLM and BD populations. The thesis begins with a short introduction, which describes the fundamental properties of brown dwarfs, relates research in this field to other areas of astronomy, and summarises the project
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Books on the topic "Low mass stars. Dwarf stars"

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Reid, I. Neill. New light on dark stars: Red dwarfs, low-mass stars, brown dwarfs. Springer, 2000.

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Howell, Steve B. On the existence of low-luminosity cataclysmic variables beyond the orbital period minimum. National Aeronautics and Space Administration, 1997.

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Howell, Steve B. On the existence of low-luminosity cataclysmic variables beyond the orbital period minimum. National Aeronautics and Space Administration, 1997.

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Howell, Steve B. On the existence of low-luminosity cataclysmic variables beyond the orbital period minimum. National Aeronautics and Space Administration, 1997.

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K, Dupree Andrea, Lago, M. T. V. T., and North Atlantic Treaty Organization. Scientific Affairs Division., eds. Formation and evolution of low mass stars. Kluwer Academic Publishers, 1988.

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Dupree, A. K., and M. T. V. T. Lago, eds. Formation and Evolution of Low Mass Stars. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3037-7.

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Prusti, Timo Juhani. Infrared studies of low mass formation. Rijksuniversiteit Groningen, 1992.

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Reipurth, Bo, and Claude Bertout, eds. Herbig-Haro Flows and the Birth of Low Mass Stars. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5608-0.

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Landsman, Wayne. The white-dwarf companions of 56 Persei and HR 3643. National Aeronautics and Space Administration, 1996.

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Landsman, Wayne. The white-dwarf companions of 56 Persei and HR 3643. National Aeronautics and Space Administration, 1996.

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Book chapters on the topic "Low mass stars. Dwarf stars"

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Nelson, Lorne A. "Low-Mass Stars and Brown Dwarfs." In Baryonic Dark Matter. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0565-8_4.

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Cameron, A. Collier, and R. D. Robinson. "Coronal Mass Ejections from a Rapidly-Rotating K0 Dwarf Star." In Formation and Evolution of Low Mass Stars. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3037-7_26.

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Reid, I. Neill, and Suzanne L. Hawley. "Observational properties of low-mass dwarfs." In New Light on Dark Stars. Springer London, 2000. http://dx.doi.org/10.1007/978-1-4471-3663-7_2.

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Kumar, Shiv S. "Very Low Mass Stars, Black Dwarfs and Planets." In Planetary Systems: Formation, Evolution, and Detection. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1154-6_7.

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Sion, Edward M., and Christian J. Ready. "Outbursts by Low-Mass White Dwarfs in Symbiotic Variables." In Evolutionary Processes in Interacting Binary Stars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2542-0_67.

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Reid, I. Neill, and Suzanne L. Hawley. "The structure, formation and evolution of low-mass stars and brown dwarfs." In New Light on Dark Stars. Springer London, 2000. http://dx.doi.org/10.1007/978-1-4471-3663-7_3.

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De Marchi, Guido, Francesco Paresce, and Martino Romaniello. "Low Mass Stars and White Dwarfs in NGC 6397." In Stellar Populations. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0125-7_82.

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Stamatellos, Dimitris. "The Formation of Low-Mass Stars and Brown Dwarfs." In The Labyrinth of Star Formation. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-03041-8_3.

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Eislöffel, Jochen, and Alexander Scholz. "Variability and Rotation in Low Mass Stars and Brown Dwarfs." In The Origins of Stars and Planets: The VLT View. Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-40277-1_27.

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Kirkpatrick, J. Davy, Michael F. Skrutskie, James Liebert, et al. "Searching for Low-Mass Stars and Brown Dwarfs with 2MASS." In The Impact of Near-Infrared Sky Surveys on Galactic and Extragalactic Astronomy. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5026-2_14.

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Conference papers on the topic "Low mass stars. Dwarf stars"

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Classen, L., S. Geier, U. Heber, S. J. O’Toole, Klaus Werner, and T. Rauch. "RV survey of low-mass companions to sdB stars." In 17TH EUROPEAN WHITE DWARF WORKSHOP. AIP, 2010. http://dx.doi.org/10.1063/1.3527814.

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Lin, Douglas N. C. "Formation of low mass stars and brown dwarfs." In The seventh astrophysical conference: Star formation, near and far. AIP, 1997. http://dx.doi.org/10.1063/1.52786.

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Liu, Michael C., Keivan G. Stassun, France Allard, et al. "Fundamental Properties of Low-Mass Stars and Brown Dwarfs." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099100.

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Stamatellos, Dimitris, Anthony P. Whitworth, and Eric Stempels. "The formation of brown dwarfs and low-mass stars by disc fragmentation." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099172.

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Rodríguez-Ledesma, Maria V., Reinhard Mundt, Jochen Eislöffel, William Herbst, and Eric Stempels. "Rotational studies of very low mass stars and brown dwarfs in the Orion Nebula Cluster." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099080.

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Cody, Ann Marie, Richard J. Stancliffe, Guenter Houdek, Rebecca G. Martin, and Christopher A. Tout. "A Search for Pulsation in Very Low-mass Stars and Brown Dwarfs." In UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP, 2007. http://dx.doi.org/10.1063/1.2818960.

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Luhman, K. L., and Eric Stempels. "Studying Planet Formation around Low-Mass Stars and Brown Dwarfs through Observations of their Circumstellar Disks." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099173.

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Rice, Emily L., Travis S. Barman, Ian S. McLean, L. Prato, J. Davy Kirkpatrick, and Eric Stempels. "Determining the Physical Properties of Very-Low-Mass Stars and Brown Dwarfs in the Near-Infrared." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099089.

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Gallardo, J., I. Baraffe, G. Chabrier, and Eric Stempels. "Evolution of very low mass pre-main sequence stars and young brown dwarfs under accretion A phenomenological approach." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099110.

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Wierling, August. "Screening correction to nuclear reaction rates in brown dwarfs and low-mass stars." In 11th Symposium on Nuclei in the Cosmos. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.100.0135.

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