Herschel-SPIRE observations of the disturbed galaxy NGC 4438
dc.contributor.author | Cortese, L. | |
dc.contributor.author | Bendo, G. J. | |
dc.contributor.author | Boselli, A. | |
dc.contributor.author | Davies, J. I. | |
dc.contributor.author | Gomez, H. L. | |
dc.contributor.author | Pohlen, M. | |
dc.contributor.author | Auld, R. | |
dc.contributor.author | Baes, M. | |
dc.contributor.author | Bock, J. J. | |
dc.contributor.author | Bradford, M. | |
dc.contributor.author | Buat, V. | |
dc.contributor.author | Castro-Rodriguez, N. | |
dc.contributor.author | Chanial, P. | |
dc.contributor.author | Charlot, S. | |
dc.contributor.author | Ciesla, L. | |
dc.contributor.author | Clements, D. L. | |
dc.contributor.author | Cooray, A. | |
dc.contributor.author | Cormier, D. | |
dc.contributor.author | Dwek, E. | |
dc.contributor.author | Eales, S. A. | |
dc.contributor.author | Elbaz, D. | |
dc.contributor.author | Galametz, M. | |
dc.contributor.author | Galliano, F. | |
dc.contributor.author | Gear, W. K. | |
dc.contributor.author | Glenn, J. | |
dc.contributor.author | Griffin, M. | |
dc.contributor.author | Hony, S. | |
dc.contributor.author | Isaak, K. G. | |
dc.contributor.author | Levenson, L. R. | |
dc.contributor.author | Lu, N. | |
dc.contributor.author | Madden, S. | |
dc.contributor.author | O'Halloran, B. | |
dc.contributor.author | Okumura, K. | |
dc.contributor.author | Oliver, S. | |
dc.contributor.author | Page, M. J. | |
dc.contributor.author | Panuzzo, P. | |
dc.contributor.author | Papageorgiou, A. | |
dc.contributor.author | Parkin, T. J. | |
dc.contributor.author | Perez-Fournon, I. | |
dc.contributor.author | Rangwala, N. | |
dc.contributor.author | Rigby, E. E. | |
dc.contributor.author | Roussel, H. | |
dc.contributor.author | Rykala, A. | |
dc.contributor.author | Sacchi, N. | |
dc.contributor.author | Sauvage, M. | |
dc.contributor.author | Schulz, B. | |
dc.contributor.author | Schirm, M. R. P. | |
dc.contributor.author | Smith, M. W. L. | |
dc.contributor.author | Spinoglio, L. | |
dc.contributor.author | Stevens, Jason | |
dc.contributor.author | Srinivasan, S. | |
dc.contributor.author | Symeonidis, M. | |
dc.contributor.author | Trichas, M. | |
dc.contributor.author | Vaccari, M. | |
dc.contributor.author | Vigroux, L. | |
dc.contributor.author | Wilson, C. D. | |
dc.contributor.author | Wozniak, H. | |
dc.contributor.author | Wright, G. S. | |
dc.contributor.author | Zeilinger, W. W. | |
dc.date.accessioned | 2012-01-31T10:01:08Z | |
dc.date.available | 2012-01-31T10:01:08Z | |
dc.date.issued | 2010-07-01 | |
dc.identifier.citation | Cortese , L , Bendo , G J , Boselli , A , Davies , J I , Gomez , H L , Pohlen , M , Auld , R , Baes , M , Bock , J J , Bradford , M , Buat , V , Castro-Rodriguez , N , Chanial , P , Charlot , S , Ciesla , L , Clements , D L , Cooray , A , Cormier , D , Dwek , E , Eales , S A , Elbaz , D , Galametz , M , Galliano , F , Gear , W K , Glenn , J , Griffin , M , Hony , S , Isaak , K G , Levenson , L R , Lu , N , Madden , S , O'Halloran , B , Okumura , K , Oliver , S , Page , M J , Panuzzo , P , Papageorgiou , A , Parkin , T J , Perez-Fournon , I , Rangwala , N , Rigby , E E , Roussel , H , Rykala , A , Sacchi , N , Sauvage , M , Schulz , B , Schirm , M R P , Smith , M W L , Spinoglio , L , Stevens , J , Srinivasan , S , Symeonidis , M , Trichas , M , Vaccari , M , Vigroux , L , Wilson , C D , Wozniak , H , Wright , G S & Zeilinger , W W 2010 , ' Herschel-SPIRE observations of the disturbed galaxy NGC 4438 ' , Astronomy and Astrophysics , vol. 518 , L63 . https://doi.org/10.1051/0004-6361/201014547 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | Bibtex: urn:35b5ad50a1b5ec1c15e900a203564959 | |
dc.identifier.other | ORCID: /0000-0002-4010-8310/work/62747679 | |
dc.identifier.uri | http://hdl.handle.net/2299/7752 | |
dc.description.abstract | We present Herschel-SPIRE observations of the perturbed galaxy NGC 4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4–5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped atomic and molecular hydrogen, supporting the idea that gas and dust are perturbed in a similar fashion by the cluster environment. Interestingly, the extra-planar dust lacks a warm temperature component when compared to the material still present in the disk, explaining why it was missed by previous far-infrared investigations. Our study provides evidence for dust stripping in clusters of galaxies and illustrates the potential of Herschel data for our understanding of environmental effects on galaxy evolution. | en |
dc.format.extent | 5 | |
dc.format.extent | 955130 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy and Astrophysics | |
dc.subject | galaxies: evolution, galaxies: individual: NGC 4438, infrared: galaxies, dust, extinction | |
dc.title | Herschel-SPIRE observations of the disturbed galaxy NGC 4438 | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1051/0004-6361/201014547 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |