Issue |
A&A
Volume 518, July-August 2010
Herschel: the first science highlights
|
|
---|---|---|
Article Number | L50 | |
Number of page(s) | 4 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201014533 | |
Published online | 16 July 2010 |
Letter to the Editor
The Herschel Virgo Cluster Survey*
III. A constraint on dust grain lifetime in early-type galaxies
1
INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy e-mail: marcel.clemens@oapd.inaf.it
2
Institut d'Astrophysique Spatiale (IAS), Bâtiment 121, Université Paris-Sud 11 and CNRS, 91405 Orsay, France e-mail: Anthony.Jones@ias.u-psud.fr
3
SISSA-ISAS, International School for Advanced Studies, via Beirut 4, 34014 Trieste, Italy
4
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, 9000 Gent, Belgium
5
Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK
6
INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy
7
Astronomical Institute, Ruhr-University Bochum, Universitaetsstr. 150, 44780 Bochum, Germany
8
Laboratoire d'Astrophysique de Marseille, UMR 6110 CNRS, 38 rue F. Joliot-Curie, 13388 Marseille, France
9
Department of Physics and Astronomy, Cardiff University, The Parade, Cardiff, CF24 3AA, UK
10
NASA Herschel Science Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA
11
ESO, Alonso de Cordova 3107, Vitacura, Santiago, Chile
12
Università di Milano-Bicocca, piazza della Scienza 3, 20100, Milano, Italy
13
CAAUL, Observatório Astronómico de Lisboa, Universidade de Lisboa,
Tapada da Ajuda, 1349-018, Lisboa, Portugal
14
Laboratoire AIM, CEA/DSM – CNRS – Université Paris Diderot, Irfu/Service d'Astrophysique, 91191 Gif sur Yvette, France
15
Max-Planck-Institut fuer extraterrestrische Physik, Giessenbachstrasse, Postfach 1312, 85741, Garching, Germany
16
INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, via Fosso del Cavaliere 100, 00133, Roma, Italy
17
Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
18
National Observatory of Athens, I. Metaxa and Vas. Pavlou, P. Penteli, 15236 Athens, Greece
19
Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, 69117 Heidelberg, Germany
Received:
29
March
2010
Accepted:
30
April
2010
Passive early-type galaxies (ETGs) provide an ideal laboratory for studying the interplay between dust formation around evolved stars and its subsequent destruction in a hot gas. Using Spitzer-IRS and Herschel data we compare the dust production rate in the envelopes of evolved AGB stars with a constraint on the total dust mass. Early-type galaxies which appear to be truly passively evolving are not detected by Herschel. We thus derive a distance independent upper limit to the dust grain survival time in the hostile environment of ETGs of <46±25 Myr for amorphous silicate grains. This implies that ETGs which are detected at far-infrared wavelengths have acquired a cool dusty medium via interaction. Given likely time-scales for ram-pressure stripping, this also implies that only galaxies with dust in a cool (atomic) medium can release dust into the intra-cluster medium.
Key words: galaxies: elliptical and lenticular, cD / galaxies: ISM / infrared: galaxies
© ESO, 2010
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