The Herschel Virgo Cluster Survey II. Truncated dust disks in HI-deficient spirals

被引：98

作者：

Cortese, L. ^{[1
]}

Davies, J. I. ^{[1
]}

Pohlen, M. ^{[1
]}

Baes, M. ^{[2
]}

Bendo, G. J. ^{[3
]}

Bianchi, S. ^{[4
]}

Boselli, A. ^{[5
]}

De Looze, I. ^{[2
]}

Fritz, J. ^{[2
]}

Verstappen, J. ^{[2
]}

Bomans, D. J. ^{[6
]}

Clemens, M. ^{[7
]}

Corbelli, E. ^{[4
]}

Dariush, A. ^{[1
]}

Alighieri, S. di Serego ^{[4
]}

Fadda, D. ^{[8
]}

Garcia-Appadoo, D. A. ^{[9
]}

Gavazzi, G. ^{[10
]}

Giovanardi, C. ^{[4
]}

Grossi, M. ^{[11
]}

Hughes, T. M. ^{[1
]}

Hunt, L. K. ^{[4
]}

Jones, A. P. ^{[12
,13
]}

Madden, S. ^{[14
]}

Pierini, D. ^{[15
]}

Sabatini, S. ^{[16
]}

Smith, M. W. L. ^{[1
]}

Vlahakis, C. ^{[17
]}

Xilouris, E. M. ^{[18
]}

Zibetti, S. ^{[19
]}

机构：

[1] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[2] Univ Ghent, Sterrenkundig Observatorium, B-9000 Ghent, Belgium

[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England

[4] INAF Osservatorio Astrofis Arcetri, I-50125 Florence, Italy

[5] Ruhr Univ Bochum, Astron Inst, D-44780 Bochum, Germany

[6] CNRS, UMR 6110, Lab Astrophys Marseille, F-13388 Marseille, France

[7] INAF Osservatorio Astron Padova, I-35122 Padua, Italy

[8] CALTECH, NASA Herschel Sci Ctr, Pasadena, CA 91125 USA

[9] ESO, Santiago, Chile

[10] Univ Milano Bicocca, I-20100 Milan, Italy

[11] Univ Lisbon, Observ Astron Lisboa, CAAUL, P-1349018 Lisbon, Portugal

[12] CNRS, F-91405 Orsay, France

[13] Univ Paris 11, IAS, F-91405 Orsay, France

[14] Univ Paris Diderot, CEA DSM CNRS, Lab AIM, Irfu Serv Astrophys, F-91191 Gif Sur Yvette, France

[15] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

[16] INAF Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy

[17] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[18] Natl Observ Athens, Inst Astron & Astrophys, Athens 15236, Greece

[19] Max Planck Inst Astron, D-69117 Heidelberg, Germany

来源：

ASTRONOMY & ASTROPHYSICS | 2010年 / 518卷

关键词：

galaxies: evolution; galaxies: clusters: individual: Virgo; infrared: galaxies; dust; extinction; LATE-TYPE GALAXIES; STAR-FORMATION; NEUTRAL HYDROGEN; ATOMIC GAS; EMISSION; SAMPLE;

D O I：

10.1051/0004-6361/201014550

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

By combining Herschel-SPIRE observations obtained as part of the Herschel Virgo Cluster Survey with 21 cm HI data from the literature, we investigate the role of the cluster environment on the dust content of Virgo spiral galaxies. We show for the first time that the extent of the dust disk is significantly reduced in HI-deficient galaxies, following remarkably well the observed "truncation" of the HI disk. The ratio of the submillimetre-to-optical diameter correlates with the HI-deficiency, suggesting that the cluster environment is able to strip dust as well as gas. These results provide important insights not only into the evolution of cluster galaxies but also into the metal enrichment of the intra-cluster medium.

引用

页数：5

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