The M 16 molecular complex under the influence of NGC 6611: Herschel 's perspective of the heating effect on the Eagle Nebula

Astronomy and Astrophysics

Volumn 542, Issue , 2012, Pages

  Hill, T ^a   Motte, F ^a   Didelon, P ^a   White, G J ^b,c   Marston, A P ^d   Nguyen Luong Q ^a   Bontemps, S ^e   André, Ph ^a   Schneider, N ^a   Hennemann, M ^a   Sauvage, M ^a   Di Francesco, J ^f   Minier, V ^a   Anderson, L D ^g   Bernard, J P ^h   Elia, D ⁱ   Griffin, M J ^j   Li, J Z ^k   Peretto, N ^a   Pezzuto, S ⁱ   Polychroni, D ⁱ   Roussel, H ^l   Rygl, K L J ⁱ   Schisano, E ⁱ   Sousbie, T ^l   Testi, L ^m   Ward Thompson, D ^j,n   Zavagno, A ^o   more..

^a STATION DE RADIOASTRONOMIE DE NANÇAY   (France)

^b RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^c OPEN UNIVERSITY   (United Kingdom)

^d EUROPEAN SPACE AGENCY   (Spain)

^e OBSERVATOIRE DE BORDEAUX   (France)

^f NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^g WEST VIRGINIA UNIVERSITY   (United States)

^h IRAP   (France)

ⁱ IAPS   (Italy)

^j CARDIFF UNIVERSITY   (United Kingdom)

^k CHINESE ACADEMY OF SCIENCES   (China)

^l INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^m EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁿ UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^o CNRS   (France)

more..

Author keywords

Dust, extinction; ISM: clouds; ISM: structure; Stars: early type; Stars: protostars

Indexed keywords

DUST , EXTINCTION; ISM : CLOUDS; ISM: STRUCTURE; STARS: EARLY-TYPE; STARS: PROTOSTARS;

DUST;

STARS;

EID: 84862643565     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219009     Document Type: Article

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