A Herschel PACS and SPIRE study of the dust content of the Cassiopeia A supernova remnant

Astronomy and Astrophysics

Volumn 518, Issue 4, 2010, Pages

  Barlow, M J ^a   Krause, O ^b   Swinyard, B M ^c   Sibthorpe, B ^d   Besel, M A ^b   Wesson, R ^a   Ivison, R J ^d   Dunne, L ^e   Gear, W K ^f   Gomez, H L ^f   Hargrave, P C ^f   Henning, Th ^b   Leeks, S J ^c   Lim, T L ^c   Olofsson, G ^g   Polehampton, E T ^c,h  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^d UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^e UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^f CARDIFF UNIVERSITY   (United Kingdom)

^g STOCKHOLM UNIVERSITY   (Sweden)

^h UNIVERSITY OF LETHBRIDGE   (Canada)

Author keywords

dust, extinction; infrared: ISM; ISM: supernova remnants

Indexed keywords

ANGULAR RESOLUTION; DUST , EXTINCTION; DUST CONTENT; HERSCHEL; HERSCHEL SPACE OBSERVATORIES; INFRARED: ISM; INTERSTELLAR DUST; ISM: SUPERNOVA REMNANTS; NONTHERMAL; NONTHERMAL EMISSION; SHOCK REGION; SPITZER; SUPERNOVA REMNANTS;

ASTRONOMY; OBSERVATORIES; TOWERS;

DUST;

EID: 77957833238     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: None     Document Type: Article

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