[Accepted Article Manuscript Version (Postprint)] Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limit†

Kevin R. Covey; Thomas P. Greene; Greg W. Doppmann; Charles J. Lada; Bruce A. Wilking

doi:10.1002/asna.200510462

[Accepted Article Manuscript Version (Postprint)] Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limit†

Kevin R. Covey, Thomas P. Greene, Greg W. Doppmann, Charles J. Lada, Bruce A. Wilking

University of Missouri-St. Louis

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	Astronomische Nachrichten
Volume	326
DOIs	https://doi.org/10.1002/asna.200510462
State	Published - Jan 12 2005

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Physics
Astrophysics and Astronomy

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@article{ef0269136fe34c59b0841904ef70775b,

title = "[Accepted Article Manuscript Version (Postprint)] Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limit†",

author = "Covey, \{Kevin R.\} and Greene, \{Thomas P.\} and Doppmann, \{Greg W.\} and Lada, \{Charles J.\} and Wilking, \{Bruce A.\}",

note = "Recent observations of nearby star forming regions have offered evidence that young brown dwarfs undergo a period of mass accretion analogous to the T Tauri phase observed in young stars. Brown dwarf analogs to stellar protostars, however, have yet to be definitively observed.",

year = "2005",

month = jan,

day = "12",

doi = "10.1002/asna.200510462",

language = "American English",

volume = "326",

journal = "Astronomische Nachrichten",

}

TY - JOUR

T1 - [Accepted Article Manuscript Version (Postprint)] Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limit†

AU - Covey, Kevin R.

AU - Greene, Thomas P.

AU - Doppmann, Greg W.

AU - Lada, Charles J.

AU - Wilking, Bruce A.

N1 - Recent observations of nearby star forming regions have offered evidence that young brown dwarfs undergo a period of mass accretion analogous to the T Tauri phase observed in young stars. Brown dwarf analogs to stellar protostars, however, have yet to be definitively observed.

PY - 2005/1/12

Y1 - 2005/1/12

UR - https://arxiv.org/abs/astro-ph/0510153

U2 - 10.1002/asna.200510462

DO - 10.1002/asna.200510462

M3 - Article

VL - 326

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

ER -

[Accepted Article Manuscript Version (Postprint)] Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limit†

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