Mg i emission lines at 12 and 18 μm in K giants

Astronomy and Astrophysics

Volumn 486, Issue 3, 2008, Pages 985-993

  Sundqvist, J O ^a   Ryde, N ^b,c   Harper, G M ^d   Kruger, A ^e,f   Richter, M J ^e,f  

^a UNIVERSITY OF MUNICH   (Germany)

^b UPPSALA UNIVERSITY   (Sweden)

^c LUND UNIVERSITY   (Sweden)

^d UNIVERSITY OF COLORADO   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f Infrared Telescope Facility

Author keywords

Line: formation; Stars: atmospheres; Stars: individual: Aldebaran; Stars: individual: Arcturus; Stars: individual: Pollux; Stars: late type

Indexed keywords

ASTROPHYSICS; ATMOSPHERIC SPECTRA; ATOMIC PHYSICS; ATOMS; CALCIUM; CHEMICAL ELEMENTS; CODES (STANDARDS); CODES (SYMBOLS); ELECTROMAGNETIC WAVE EMISSION; EMISSION SPECTROSCOPY; HYDROGEN; LIGHT METALS; MAGNESIUM; MAGNESIUM PRINTING PLATES; MAGNETIC FIELDS; NONMETALS; RADIATIVE TRANSFER; SILICON; SOLAR ENERGY; SPACE PROBES; STANDARDS; STARS; TRACE ELEMENTS;

ATOMIC DATA; EMISSION LINES; ENERGY LEVELS; EVOLVED STARS; HIGH RESOLUTIONS; LINE PROFILES; LINE SPECTRUM; MID-INFRARED (MIR); NEUTRAL HYDROGEN; NON LTE; ONE-DIMENSIONAL; PROCYON; RADIATIVE TRANSFER CODES; SPECTRA (CO); STATISTICAL EQUILIBRIUM; STELLAR ATMOSPHERES; STELLAR MAGNETIC FIELDS;

CURVE FITTING;

EID: 47749104525     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809778     Document Type: Article

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