Early-type stars observed in the ESO UVES Paranal Observatory Project - III. Sub-parsec and au-scale structure in the interstellar medium

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 1, 2011, Pages 59-75

  Smoker, J V ^a   Bagnulo, S ^b   Cabanac, R ^c   Keenan, F P ^d   Fossati, L ^e,f   Ledoux, C ^a   Jehin, E ^g   Melo, C ^h  

^a EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^b ARMAGH OBSERVATORY   (United Kingdom)

^c OBSERVATOIRE MIDI PYRÉNÉES   (France)

^d QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^e UNIVERSITY OF VIENNA   (Austria)

^f OPEN UNIVERSITY   (United Kingdom)

^g UNIVERSITY OF LIÈGE   (Belgium)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

ISM: abundances; ISM: structure; Open clusters and associations: individual: IC2391 (OmniVel); Open clusters and associations: individual: NGC6475 (M7); Open clusters and associations: individual: Praesepe (M44); Stars: early type

Indexed keywords

IODINE COMPOUNDS; OBSERVATORIES; SIGNAL TO NOISE RATIO; STARS;

INTERSTELLAR MEDIAS; INTERSTELLAR MEDIUM: ABUNDANCES; INTERSTELLAR MEDIUM: STRUCTURE; MEDIA STRUCTURE; OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: IC2391 (OMNIVEL); OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: NGC6475 (M7); OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: PRAESEPE (M44); OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; STARS:EARLY TYPE;

GEOMETRICAL OPTICS;

EID: 79957883834     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.17987.x     Document Type: Article

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