A pulsational approach to near-infrared and visual magnitudes of RR Lyr stars

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 4, 2003, Pages 1097-1106

  Bono, G ^a   Caputo, F ^a   Castellani, V ^a,b   Marconi, M ^c   Storm, J ^d   Degl'Innocenti, S ^e  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b INFN SEZIONE DI FERRARA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^d ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^e UNIVERSITY OF PISA   (Italy)

Author keywords

Globular clusters: general; Stars: evolution; Stars: horizontal branch; Stars: oscillations; Stars: variables: other

Indexed keywords

ASTROPHYSICS; CALIBRATION; GEOMETRICAL OPTICS; INFRARED DEVICES; METALS; RELIABILITY THEORY; STARS;

GLOBULAR CLUSTERS:GENERAL; METAL CONTENT; NEAR INFRARED; NEAR-INFRARED; STAR OSCILLATIONS; STAR: EVOLUTION; STAR: VARIABLE: OTHER; STARS: HORIZONTAL BRANCH; STARS: VARIABLES; VISUAL MAGNITUDES;

LUMINANCE;

EID: 0142198890     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06878.x     Document Type: Article

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