On the distance, reddening and progenitor of V838 Mon

Astronomy and Astrophysics

Volumn 434, Issue 3, 2005, Pages 1107-1116

  Munari, U ^a   Henden, A ^b   Vallenari, A ^a   Bond, H E ^c   Corradi, R L M ^d   Crause, L ^e   Desidera, S ^a   Giro, E ^a   Marrese, P M ^a   Ragaini, S ^a   Siviero, A ^a   Sordo, R ^a   Starrfield, S ^f   Tomov, T ^g   Villanova, S ^h   Zwitter, T ⁱ   Wagner, R M ^j  

^a INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^b UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^c STScI   (United States)

^d ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^e SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^f ARIZONA STATE UNIVERSITY   (United States)

^g NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^h UNIVERSITY OF PADOVA   (Italy)

ⁱ UNIVERSITY OF LJUBLJANA   (Slovenia)

^j UNIVERSITY OF ARIZONA   (United States)

more..

Author keywords

ISM: lines and bands; Stars: early type; Stars: evolution; Stars: individual: V838 Mon; Stars: peculiar; Stars: winds, outflows

Indexed keywords

CARBON; GALAXIES; INFRARED RADIATION; KINEMATICS; ORBITS; SPECTROPHOTOMETRY; SPECTROSCOPIC ANALYSIS; WIND;

EARLY-TYPE - STARS; EVOLUTION - STARS; INDIVIDUAL; LINES AND BANDS - STARS; PECULIAR; STARS; V838 MON - STARS; WINDS, OUTFLOWS - ISM;

ASTRONOMY;

EID: 21044454997     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041751     Document Type: Article

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