An Infrared Spectral Sequence for M Dwarfs

H.R.A. Jones; A.J. Longmore; R.F. Jameson

An Infrared Spectral Sequence for M Dwarfs

H.R.A. Jones, A.J. Longmore, R.F. Jameson

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Abstract

We present a spectral sequence from 1-2.5 um of M dwarfs from GL411 which is classified as M2V to the best brown dwarf candidate GD165B (M10V). This sequence shows the progressive importance of water vapour in the stmospheres of M dwarfs. We take the strength of the water absorption bands as the basis of a new method to derive effective temperatures. We also identify many of the stronger atomic and molecular features and find that their strengths correlate with our derived temperature scale.

Original language	English
Title of host publication	In: Cool Stars, Stellar Systems and the Sun; Eighth Cambridge Workshop - ASP Conf Series 64
Publisher	Astronomical Society of the Pacific
Pages	614-8
ISBN (Print)	0-937707-83-X
Publication status	Published - 1994

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@inproceedings{6eb79fbeba3a4597b7644d2b7c4610a0,

title = "An Infrared Spectral Sequence for M Dwarfs",

abstract = "We present a spectral sequence from 1-2.5 um of M dwarfs from GL411 which is classified as M2V to the best brown dwarf candidate GD165B (M10V). This sequence shows the progressive importance of water vapour in the stmospheres of M dwarfs. We take the strength of the water absorption bands as the basis of a new method to derive effective temperatures. We also identify many of the stronger atomic and molecular features and find that their strengths correlate with our derived temperature scale.",

author = "H.R.A. Jones and A.J. Longmore and R.F. Jameson",

note = "Original paper can be found at: http://www.astrosociety.org/pubs/cs/035-069.html--Copyright Astronomical Society of the Pacific",

year = "1994",

language = "English",

isbn = "0-937707-83-X",

pages = "614--8",

booktitle = "In: Cool Stars, Stellar Systems and the Sun; Eighth Cambridge Workshop - ASP Conf Series 64",

publisher = "Astronomical Society of the Pacific",

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TY - GEN

T1 - An Infrared Spectral Sequence for M Dwarfs

AU - Jones, H.R.A.

AU - Longmore, A.J.

AU - Jameson, R.F.

N1 - Original paper can be found at: http://www.astrosociety.org/pubs/cs/035-069.html--Copyright Astronomical Society of the Pacific

PY - 1994

Y1 - 1994

N2 - We present a spectral sequence from 1-2.5 um of M dwarfs from GL411 which is classified as M2V to the best brown dwarf candidate GD165B (M10V). This sequence shows the progressive importance of water vapour in the stmospheres of M dwarfs. We take the strength of the water absorption bands as the basis of a new method to derive effective temperatures. We also identify many of the stronger atomic and molecular features and find that their strengths correlate with our derived temperature scale.

AB - We present a spectral sequence from 1-2.5 um of M dwarfs from GL411 which is classified as M2V to the best brown dwarf candidate GD165B (M10V). This sequence shows the progressive importance of water vapour in the stmospheres of M dwarfs. We take the strength of the water absorption bands as the basis of a new method to derive effective temperatures. We also identify many of the stronger atomic and molecular features and find that their strengths correlate with our derived temperature scale.

M3 - Conference contribution

SN - 0-937707-83-X

SP - 614

EP - 618

BT - In: Cool Stars, Stellar Systems and the Sun; Eighth Cambridge Workshop - ASP Conf Series 64

PB - Astronomical Society of the Pacific

ER -

An Infrared Spectral Sequence for M Dwarfs

Abstract

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