The abundance of brown dwarfs by Binney, J

The abundance of brown dwarfs by Binney, J

Stellar and Brown Dwarf Astronomy / by Rinehart, Micheal, author 650305, Mallory, Eusebio, author 650306

BROWN DWARFS: MYSTERY AND SHOW by Ya. V. Pavlenko

“…Results of the numerical simulation of the spectrum of the brown dwarf candidate Teide 1 discovered by Rebolo et al. (1995) are discussed.…”
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Young brown dwarfs in Orion by Riddick, F, Roche, P, Lucas, P

Modelling the Spectra of Brown Dwarfs by Garland, R

“…Brown dwarfs (BDs) are substellar mass objects with masses ≤80M_<em>Jup</em>, the hydrogenburning limit. …”

The current population of benchmark brown dwarfs by Clarke J.R.A., Gallardo J., Gálvez-Ortiz M.C., Jones H.R.A., Zhang Z.H., Burningham B., Ruiz M.T., Day-Jones A.C., Pinfield D.J., Jenkins J.S.

“…The number of brown dwarfs (BDs) now identified tops 700. Yet our understanding of these cool objects is still lacking, and models are struggling to accurately reproduce observations. …”
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Brown dwarfs in wide-field surveys by Lodieu N.

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Brown dwarfs in retrogradely precessing cataclysmic variables? by Martin E.L., Deshpande R., Montgomery M.M.

“…Assuming the primary does not accrete much of the mass lost from the secondary, we identify the theoretical low mass star/brown dwarf boundary. We find no observational candidates in our study that could qualify as brown dwarfs.…”
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Cloud-convection feedback in brown dwarf atmospheres by Lefevre, M, Tan, X, Lee, EKH, Pierrehumbert, RT

“…<p>Numerous observational evidence has suggested the presence of active meteorology in the atmospheres of brown dwarfs. A near-infrared brightness variability has been observed. …”

Spectroscopy of planetary mass brown dwarfs in Orion by Lucas, P, Weights, D, Roche, P, Riddick, F

Periodic variability of the brown dwarf Kelu-1 by Clarke, F, Tinney, C, Hodgkin, S

Optical Spectroscopy of young brown dwarfs in Orion by Riddick, F, Roche, P, Lucas, P

“…Red spectra of a sample of low-mass stars and brown dwarfs in the Orion Trapezium cluster are discussed. …”

Long-term 4.6 μm Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates by Hunter Brooks, J. Davy Kirkpatrick, Aaron M. Meisner, Christopher R. Gelino, Daniella C. Bardalez Gagliuffi, Federico Marocco, Adam C. Schneider, Jacqueline K. Faherty, S. L. Casewell, Yadukrishna Raghu, Marc J. Kuchner, The Backyard Worlds: Planet 9 Collaboration

Subjects: “…Brown dwarfs…”
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JWST/NIRSpec Observations of the Coldest Known Brown Dwarf by K. L. Luhman, P. Tremblin, C. Alves de Oliveira, S. M. Birkmann, I. Baraffe, G. Chabrier, E. Manjavacas, R. J. Parker, J. Valenti

Subjects: “…Brown dwarfs…”
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Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys by Kevin N. Hainline, Jakob M. Helton, Benjamin D. Johnson, Fengwu Sun, Michael W. Topping, Jarron M. Leisenring, William M. Baker, Daniel J. Eisenstein, Ryan Hausen, Raphael E. Hviding, Jianwei Lyu, Brant Robertson, Sandro Tacchella, Christina C. Williams, Christopher N. A. Willmer, Thomas L. Roellig

Subjects: “…Brown dwarfs…”
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DEPLETION OF TiO AND SPECTRA OF THE COOLEST BROWN DWARFS by Ya. V. Pavlenko

“…This study was performed in the context of the ”lithium test” for brown dwarfs proposed by Rebolo et al. (1992). We consider the formation of lithium dust species in atmospheres of the coolest stars and substellar objects. …”
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DISCOVERY OF A CANDIDATE FOR THE COOLEST KNOWN BROWN DWARF by Luhman, K. L., Bochanski, John J., Burgasser, Adam J.

“…Therefore, the companion could be either a brown dwarf that formed like a binary star or a giant planet that was born within a disk and has been dynamically scattered to a larger orbit.…”
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Atmospheric dynamics of hot giant planets and brown dwarfs by Showman, AP, Tan, X, Parmentier, V

“…Finally, irradiated brown dwarfs help to bridge the gap between these classes of objects, experiencing intense external irradiation as well as vigorous interior convection. …”

A deep survey of brown dwarfs in Orion with Gemini by Lucas, P, Roche, P, Tamura, M

“…Only 33 of the brown dwarf candidates are planetary mass candidates with estimated masses in the range 0.003 &lt; M &lt; 0.012 M ⊙. …”