A new model for the infrared brightness of the galaxy

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 2, 2000, Pages 263-270

  Lepine J R D ^a   Leroy, P ^b  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b PONTIFICAL CATHOLIC UNIVERSITY OF MINAS GERAIS   (Brazil)

Author keywords

Galaxy: kinematics and dynamics; Galaxy: stellar content; Galaxy: Structure

Indexed keywords

COSMOLOGY; INFRARED DEVICES; LUMINANCE; MONTE CARLO METHODS; STARS;

BRIGHTNESS DISTRIBUTION; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY:STELLAR CONTENT; MONTECARLO METHODS; NEAR INFRARED; NEAR-INFRARED; SPACE LAB; SPIRAL ARMS; SPIRAL GALAXIES;

GALAXIES;

EID: 0038012286     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03227.x     Document Type: Article

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