Infrared spectra of hot HF and DF

R S  Ram; Z  Morbi; B  Guo; K Q  Zhang; P F  Bernath; J  VanderAuwera; J W C  Johns; S P  Davis

Infrared spectra of hot HF and DF

R S Ram, Z Morbi, B Guo, K Q Zhang, P F Bernath, J VanderAuwera, J W C Johns, S P Davis

Chemistry

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

Abstract

New Fourier transform emission measurements were obtained for HF and DF at a temperature of 2300 degrees C. Both pure rotation and vibration-rotation lines were measured with a precision of about 0.0005 c(m)(-1). These new lines were combined with previously measured data to give improved rotational constants for the vibrational levels v = 0-5. The HF molecule is the most convenient monitor of F-19 abundances in cool stars.

Original language	English
Pages (from-to)	247-254
Number of pages	8
Journal	ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume	103
Issue number	1
Publication status	Published - Mar 1996

Keywords

line, identification
methods, laboratory
molecular processes
stars, abundances
FLUORINE
LASER

Cite this

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title = "Infrared spectra of hot HF and DF",

abstract = "New Fourier transform emission measurements were obtained for HF and DF at a temperature of 2300 degrees C. Both pure rotation and vibration-rotation lines were measured with a precision of about 0.0005 c(m)(-1). These new lines were combined with previously measured data to give improved rotational constants for the vibrational levels v = 0-5. The HF molecule is the most convenient monitor of F-19 abundances in cool stars.",

keywords = "line, identification, methods, laboratory, molecular processes, stars, abundances, FLUORINE, LASER",

author = "Ram, {R S} and Z Morbi and B Guo and Zhang, {K Q} and Bernath, {P F} and J VanderAuwera and Johns, {J W C} and Davis, {S P}",

year = "1996",

month = mar,

language = "English",

volume = "103",

pages = "247--254",

journal = "ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES",

issn = "0067-0049",

publisher = "IOP Publishing",

number = "1",

}

TY - JOUR

T1 - Infrared spectra of hot HF and DF

AU - Ram, R S

AU - Morbi, Z

AU - Guo, B

AU - Zhang, K Q

AU - Bernath, P F

AU - VanderAuwera, J

AU - Johns, J W C

AU - Davis, S P

PY - 1996/3

Y1 - 1996/3

N2 - New Fourier transform emission measurements were obtained for HF and DF at a temperature of 2300 degrees C. Both pure rotation and vibration-rotation lines were measured with a precision of about 0.0005 c(m)(-1). These new lines were combined with previously measured data to give improved rotational constants for the vibrational levels v = 0-5. The HF molecule is the most convenient monitor of F-19 abundances in cool stars.

AB - New Fourier transform emission measurements were obtained for HF and DF at a temperature of 2300 degrees C. Both pure rotation and vibration-rotation lines were measured with a precision of about 0.0005 c(m)(-1). These new lines were combined with previously measured data to give improved rotational constants for the vibrational levels v = 0-5. The HF molecule is the most convenient monitor of F-19 abundances in cool stars.

KW - line, identification

KW - methods, laboratory

KW - molecular processes

KW - stars, abundances

KW - FLUORINE

KW - LASER

M3 - Article

VL - 103

SP - 247

EP - 254

JO - ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

JF - ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

SN - 0067-0049

IS - 1

ER -