Laboratory data for cool star modelling

Peter Bernath

Laboratory data for cool star modelling

Chemistry

Research output: Chapter in Book/Report/Conference proceeding › Chapter

Abstract

Recent laboratory work on water, methane and metal hydrides for simulation of spectral energy distributions of cool astronomical objects is reviewed. These molecules are found in sunspots, cool stellar atmospheres and in brown dwarfs. The calculation of opacities is discussed for CrH, FeH and TiH. New spectra of the Violet System of CN and the Swan System Of C-2 have also been analyzed.

Original language	English
Title of host publication	WHY GALAXIES CARE ABOUT AGB STARS: THEIR IMPORTANCE AS ACTORS AND PROBES
Pages	71-79
Number of pages	9
Volume	378
Publication status	Published - 2007

Publication series

Name	ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
Publisher	ASTRONOMICAL SOC PACIFIC
Volume	378

Keywords

INFRARED SPECTRUM
L-SUBDWARF
MU CEPHEI
LINE LIST
M-DWARFS
S-STARS
WATER
EMISSION
SPECTROSCOPY
ATMOSPHERES

Cite this

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title = "Laboratory data for cool star modelling",

abstract = "Recent laboratory work on water, methane and metal hydrides for simulation of spectral energy distributions of cool astronomical objects is reviewed. These molecules are found in sunspots, cool stellar atmospheres and in brown dwarfs. The calculation of opacities is discussed for CrH, FeH and TiH. New spectra of the Violet System of CN and the Swan System Of C-2 have also been analyzed.",

keywords = "INFRARED SPECTRUM, L-SUBDWARF, MU CEPHEI, LINE LIST, M-DWARFS, S-STARS, WATER, EMISSION, SPECTROSCOPY, ATMOSPHERES",

author = "Peter Bernath",

year = "2007",

language = "English",

isbn = "978-1-58381-318-8",

volume = "378",

series = "ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES",

publisher = "ASTRONOMICAL SOC PACIFIC",

pages = "71--79",

booktitle = "WHY GALAXIES CARE ABOUT AGB STARS: THEIR IMPORTANCE AS ACTORS AND PROBES",

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TY - CHAP

T1 - Laboratory data for cool star modelling

AU - Bernath, Peter

PY - 2007

Y1 - 2007

N2 - Recent laboratory work on water, methane and metal hydrides for simulation of spectral energy distributions of cool astronomical objects is reviewed. These molecules are found in sunspots, cool stellar atmospheres and in brown dwarfs. The calculation of opacities is discussed for CrH, FeH and TiH. New spectra of the Violet System of CN and the Swan System Of C-2 have also been analyzed.

AB - Recent laboratory work on water, methane and metal hydrides for simulation of spectral energy distributions of cool astronomical objects is reviewed. These molecules are found in sunspots, cool stellar atmospheres and in brown dwarfs. The calculation of opacities is discussed for CrH, FeH and TiH. New spectra of the Violet System of CN and the Swan System Of C-2 have also been analyzed.

KW - INFRARED SPECTRUM

KW - L-SUBDWARF

KW - MU CEPHEI

KW - LINE LIST

KW - M-DWARFS

KW - S-STARS

KW - WATER

KW - EMISSION

KW - SPECTROSCOPY

KW - ATMOSPHERES

M3 - Chapter

SN - 978-1-58381-318-8

VL - 378

T3 - ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES

SP - 71

EP - 79

BT - WHY GALAXIES CARE ABOUT AGB STARS: THEIR IMPORTANCE AS ACTORS AND PROBES

ER -