Granulation in K-type dwarf stars I. Spectroscopic observations

Astronomy and Astrophysics

Volumn 492, Issue 3, 2008, Pages 841-855

  Ramirez I ^a,b   Allende Prieto, C ^a   Lambert, D L ^a,c  

^a The University of Texas at Austin   (United States)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Stars: atmospheres; Stars: late type; Sun: granulation; Techniques: spectroscopic

Indexed keywords

ASTROPHYSICS; FADING (RADIO); FLUID DYNAMICS; GRANULATION; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; SANDWICH STRUCTURES; SATELLITE GROUND STATIONS; SIGNAL TO NOISE RATIO; SPECTROGRAPHS; SURFACE TESTING; TELESCOPES; VELOCITY; WAVELENGTH;

BLUE SHIFTS; BLUESHIFTED; DWARF STARS; EQUIVALENT WIDTHS; HIGH RESOLUTIONS; HYDRODYNAMIC MODELS; MCDONALD; RADIAL VELOCITIES; RESIDUAL CORES; ROTATIONAL VELOCITIES; SIGNAL-TO-NOISE RATIOS; SOLAR SPECTRUMS; SPECTROSCOPIC OBSERVATIONS; STARS: ATMOSPHERES; STELLAR ACTIVITIES; STELLAR PARAMETERS; SUN: GRANULATION; SURFACE CONVECTIONS; TECHNIQUES: SPECTROSCOPIC; WAVELENGTH SCALES; WAVELENGTH SHIFTS; ZERO POINTS;

STARS;

EID: 57649202593     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810901     Document Type: Article

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