CRIRES spectroscopy and empirical line-by-line identification of FeH molecular absorption in an M dwarf

Astronomy and Astrophysics

Volumn 523, Issue 3, 2010, Pages

  Wende, S ^a   Reiners, A ^a   Seifahrt, A ^b   Bernath, P F ^c  

^a UNIVERSITY OF GÖTTINGEN   (Germany)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF YORK   (United Kingdom)

Author keywords

line: identification; line: profiles; molecular data; stars: late type

Indexed keywords

ABSORPTION LINES; CROSS CORRELATION TECHNIQUES; EMPIRICAL LINE; ENHANCEMENT FACTOR; EQUIVALENT WIDTH; HIGH-PRECISION SPECTROSCOPY; IN-LINE; INSTRUMENTAL BROADENING; LINE DATA; LINE INTENSITIES; LINE STRENGTH; LINE: IDENTIFICATION; LINE: PROFILES; LOW-MASS STARS; MAGNETIC FIELD STRENGTHS; MODEL SPECTRA; MOLECULAR ABSORPTION; MOLECULAR DATA; OBSERVED DATA; RADIAL VELOCITY; ROTATIONAL TEMPERATURE; SCALING FACTORS; SPECTRAL REGION; STARS: LATE-TYPE; TEMPERATURE SENSITIVE; VAN DER WAALS; VIBRATIONAL BANDS; VOIGT FUNCTIONS;

ABSORPTION; ASTROPHYSICS; MAGNETIC FIELDS; NORMAL DISTRIBUTION; ROTATION; STARS; VAN DER WAALS FORCES;

ABSORPTION SPECTROSCOPY;

EID: 78449236978     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015220     Document Type: Article

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