The Herschel Virgo Cluster Survey - XVI. A cluster inventory☆

被引：18

作者：

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

Bianchi, S. ^{[2
]}

Baes, M. ^{[3
]}

Bendo, G. J. ^{[4
]}

Clemens, M. ^{[5
]}

De Looze, I. ^{[3
]}

Alighieri, S. di Serego ^{[2
]}

Fritz, J. ^{[3
]}

Fuller, C. ^{[1
]}

Pappalardo, C. ^{[6
]}

Hughes, T. M. ^{[3
]}

Madden, S. ^{[7
]}

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

Verstappen, J. ^{[3
]}

Vlahakis, C. ^{[8
]}

机构：

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

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

[3] Univ Ghent, Sterrenkundig Observ, B-9000 Ghent, Belgium

[4] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England

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

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

[7] CEA DSM CNRS Univ Paris Diderot, Irfu Serv, Lab AIM, F-91191 Paris, France

[8] Joint ALMA Observ European Southern Observ, Santiago, Chile

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2014年 / 438卷 / 03期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

galaxies: clusters: individual: Virgo; galaxies: ISM; INTRACLUSTER PLANETARY-NEBULAE; GALAXY ENVIRONMENT SURVEY; FAR-INFRARED EMISSION; STAR-FORMATION RATE; FAST ALPHA SURVEY; PHYSICAL-PROPERTIES; CHEMICAL ENRICHMENT; LUMINOSITY FUNCTION; DUST TEMPERATURES; SCALING RELATIONS;

D O I：

10.1093/mnras/stt2213

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Herschel far-infrared (FIR) observations are used to construct Virgo cluster galaxy luminosity functions and to show that the cluster lacks the very bright and the numerous faint sources detected in field galaxy surveys. The FIR spectral energy distributions are fitted to obtain dust masses and temperatures and the dust mass function. The cluster is overdense in dust by about a factor of 100 compared to the field. The same emissivity (beta)-temperature relation applies for different galaxies as that found for different regions of M31. We use optical and H i data to show that Virgo is overdense in stars and atomic gas by about a factor of 100 and 20, respectively. Metallicity values are used to measure the mass of metals in the gas phase. The mean metallicity is similar to 0.7 solar, and similar to 50 per cent of the metals are in the dust. For the cluster as a whole, the mass density of stars in galaxies is eight times that of the gas and the gas mass density is 130 times that of the metals. We use our data to consider the chemical evolution of the individual galaxies, inferring that the measured variations in the effective yield are due to galaxies having different ages, being affected to varying degrees by gas loss. Four galaxy scaling relations are considered: mass-metallicity, mass-velocity, mass-star formation rate and mass-radius - we suggest that initial galaxy mass is the prime driver of a galaxy's ultimate destiny. Finally, we use X-ray observations and galaxy dynamics to assess the dark and baryonic matter content compared to the cosmological model.

引用

页码：1922 / 1947

页数：26

共 142 条

[1] ABSORPTIVE PROPERTIES OF SILICATE CORE-MANTLE GRAINS [J].

AANNESTAD, PA .

ASTROPHYSICAL JOURNAL, 1975, 200 (01) :30-41

[2] THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY [J].

Abazajian, Kevork N. ;

Adelman-McCarthy, Jennifer K. ;

Agueros, Marcel A. ;

Allam, Sahar S. ;

Prieto, Carlos Allende ;

An, Deokkeun ;

Anderson, Kurt S. J. ;

Anderson, Scott F. ;

Annis, James ;

Bahcall, Neta A. ;

Bailer-Jones, C. A. L. ;

Barentine, J. C. ;

Bassett, Bruce A. ;

Becker, Andrew C. ;

Beers, Timothy C. ;

Bell, Eric F. ;

Belokurov, Vasily ;

Berlind, Andreas A. ;

Berman, Eileen F. ;

Bernardi, Mariangela ;

Bickerton, Steven J. ;

Bizyaev, Dmitry ;

Blakeslee, John P. ;

Blanton, Michael R. ;

Bochanski, John J. ;

Boroski, William N. ;

Brewington, Howard J. ;

Brinchmann, Jarle ;

Brinkmann, J. ;

Brunner, Robert J. ;

Budavari, Tamas ;

Carey, Larry N. ;

Carliles, Samuel ;

Carr, Michael A. ;

Castander, Francisco J. ;

Cinabro, David ;

Connolly, A. J. ;

Csabai, Istvan ;

Cunha, Carlos E. ;

Czarapata, Paul C. ;

Davenport, James R. A. ;

de Haas, Ernst ;

Dilday, Ben ;

Doi, Mamoru ;

Eisenstein, Daniel J. ;

Evans, Michael L. ;

Evans, N. W. ;

Fan, Xiaohui ;

Friedman, Scott D. ;

Frieman, Joshua A. .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2009, 182 (02) :543-558

[3] Planck early results. XXIV. Dust in the diffuse interstellar medium and the Galactic halo [J].

Abergel, A. ;

Ade, P. A. R. ;

Aghanim, N. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Baccigalupi, C. ;

Balbi, A. ;

Banday, A. J. ;

Barreiro, R. B. ;

Bartlett, J. G. ;

Battaner, E. ;

Benabed, K. ;

Benoit, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bhatia, R. ;

Blagrave, K. ;

Bock, J. J. ;

Bonaldi, A. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bucher, M. ;

Burigana, C. ;

Cabella, P. ;

Cantalupo, C. M. ;

Cardoso, J. -F. ;

Catalano, A. ;

Cayon, L. ;

Challinor, A. ;

Chamballu, A. ;

Chiang, L. -Y ;

Chiang, C. ;

Christensen, P. R. ;

Clements, D. L. ;

Colombi, S. ;

Couchot, F. ;

Coulais, A. ;

Crill, B. P. ;

Cuttaia, F. ;

Danese, L. ;

Davies, R. D. ;

Davis, R. J. ;

de Bernardis, P. ;

de Gasperis, G. ;

de Rosa, A. ;

de Zotti, G. ;

Delabrouille, J. .

ASTRONOMY & ASTROPHYSICS, 2011, 536

[4]

ARIMOTO N, 1987, ASTRON ASTROPHYS, V173, P23

[5] Narrowband imaging in [O III] and Hα to search for intracluster planetary nebulae in the Virgo Cluster [J].

Arnaboldi, M ;

Freeman, KC ;

Okamura, S ;

Yasuda, N ;

Gerhard, O ;

Napolitano, NR ;

Pannella, M ;

Ando, H ;

Doi, M ;

Furusawa, H ;

Hamabe, M ;

Kimura, M ;

Kajino, T ;

Komiyama, Y ;

Miyazaki, S ;

Nakata, F ;

Ouchi, M ;

Sekiguchi, M ;

Shimasaku, K ;

Yagi, M .

ASTRONOMICAL JOURNAL, 2003, 125 (02) :514-524

[6] Intracluster planetary nebulae in Virgo:: Photometric selection, spectroscopic validation, and cluster depth [J].

Arnaboldi, M ;

Aguerri, JAL ;

Napolitano, NR ;

Gerhard, O ;

Freeman, KC ;

Feldmeier, J ;

Capaccioli, M ;

Kudritzki, RP ;

Méndez, RH .

ASTRONOMICAL JOURNAL, 2002, 123 (02) :760-771

[7]

ARNETT D, 1991, ASTR SOC P, V20, P389

[8] On OH line formation and oxygen abundances in metal-poor stars [J].

Asplund, M ;

Pérez, AEG .

ASTRONOMY & ASTROPHYSICS, 2001, 372 (02) :601-615

[9] The Herschel Virgo Cluster Survey - XII. FIR properties of optically selected Virgo cluster galaxies [J].

Auld, R. ;

Bianchi, S. ;

Smith, M. W. L. ;

Davies, J. I. ;

Bendo, G. J. ;

Alighieri, S. di Serego ;

Cortese, L. ;

Baes, M. ;

Bomans, D. J. ;

Boquien, M. ;

Boselli, A. ;

Ciesla, L. ;

Clemens, M. ;

Corbelli, E. ;

De Looze, I. ;

Fritz, J. ;

Gavazzi, G. ;

Pappalardo, C. ;

Grossi, M. ;

Hunt, L. K. ;

Madden, S. ;

Magrini, L. ;

Pohlen, M. ;

Verstappen, J. ;

Vlahakis, C. ;

Xilouris, E. M. ;

Zibetti, S. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 428 (03) :1880-1910

[10] On the baryonic, stellar, and luminous scaling relations of disk galaxies [J].

Avila-Reese, V. ;

Zavala, J. ;

Firmani, C. ;

Hernandez-Toledo, H. M. .

ASTRONOMICAL JOURNAL, 2008, 136 (03) :1340-1360

← 1 2 3 4 5 6 7 8 9 10 →