The environmental dependence of the structure of outer galactic discs in STAGES spiral galaxies
dc.contributor.author | Maltby, David T. | en_US |
dc.contributor.author | Gray, Meghan E. | en_US |
dc.contributor.author | Aragón‐salamanca, Alfonso | en_US |
dc.contributor.author | Wolf, Christian | en_US |
dc.contributor.author | Bell, Eric F. | en_US |
dc.contributor.author | Jogee, Shardha | en_US |
dc.contributor.author | Häußler, Boris | en_US |
dc.contributor.author | Barazza, Fabio D. | en_US |
dc.contributor.author | Böhm, Asmus | en_US |
dc.contributor.author | Jahnke, Knud | en_US |
dc.date.accessioned | 2012-01-05T22:06:51Z | |
dc.date.available | 2013-03-04T15:29:55Z | en_US |
dc.date.issued | 2012-01-01 | en_US |
dc.identifier.citation | Maltby, David T.; Gray, Meghan E.; Aragón‐salamanca, Alfonso ; Wolf, Christian; Bell, Eric F.; Jogee, Shardha; Häußler, Boris ; Barazza, Fabio D.; Böhm, Asmus ; Jahnke, Knud (2012). "The environmental dependence of the structure of outer galactic discs in STAGES spiral galaxies." Monthly Notices of the Royal Astronomical Society 419(1). <http://hdl.handle.net/2027.42/89539> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/89539 | |
dc.description.abstract | We present an analysis of V ‐band radial surface brightness profiles for spiral galaxies from the field and cluster environments using Hubble Space Telescope /Advanced Camera for Surveys imaging and data from the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). We use a large sample of ∼330 face‐on to intermediately inclined spiral galaxies and assess the effect of the galaxy environment on the azimuthally averaged radial surface brightness μ profiles for each galaxy in the outer stellar disc (24 < μ < 26.5 mag arcsec −2 ). For galaxies with a purely exponential outer disc (∼50 per cent), we determine the significance of an environmental dependence on the outer disc scalelength h out . For galaxies with a broken exponential in their outer disc, either down‐bending ( truncation , ∼10 per cent) or up‐bending ( antitruncation , ∼40 per cent), we measure the strength T (outer‐to‐inner scalelength ratio, log 10 h out / h in ) of the μ breaks and determine the significance of an environmental dependence on break strength T . Surprisingly, we find no evidence to suggest any such environmental dependence on either outer disc scalelength h out or break strength T , implying that the galaxy environment is not affecting the stellar distribution in the outer stellar disc. We also find that for galaxies with small effective radii ( r e < 3 kpc) there is a lack of outer disc truncations in both the field and cluster environments. Our results suggest that the stellar distribution in the outer disc of spiral galaxies is not significantly affected by the galaxy environment. | en_US |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Galaxies: Clusters: Individual: A901/2 | en_US |
dc.subject.other | Galaxies: Evolution | en_US |
dc.subject.other | Galaxies: Spiral | en_US |
dc.subject.other | Galaxies: Structure | en_US |
dc.title | The environmental dependence of the structure of outer galactic discs in STAGES spiral galaxies | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Astronomy, University of Michigan, 830 Dennison Building, 500 Church St., Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | School of Physics and Astronomy, The University of Nottingham, University Park, Nottingham NG7 2RD | en_US |
dc.contributor.affiliationother | Department of Physics, Denys Wilkinson Building, University of Oxford, Keble Road, Oxford OX1 3RH | en_US |
dc.contributor.affiliationother | Department of Astronomy, University of Texas at Austin, 1 University Station, C1400 Austin, TX 78712‐0259, USA | en_US |
dc.contributor.affiliationother | Department of Physics, University of Basel, Klingelbergstrasse 82, 4056 Basel, Switzerland | en_US |
dc.contributor.affiliationother | Institute of Astro‐ and Particle Physics, University of Innsbruck, Technikerstr. 25/8, A‐6020 Innsbruck, Austria | en_US |
dc.contributor.affiliationother | Max‐Plank‐Institut für Astronomie, Königstuhl 17, D‐69117 Heidelberg, Germany | en_US |
dc.identifier.pmid | 17278036 | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/89539/1/j.1365-2966.2011.19727.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2011.19727.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
dc.identifier.citedreference | Azzollini R., Trujillo I., Beckman J. E., 2008, ApJ, 684, 1026 | en_US |
dc.identifier.citedreference | Bakos J., Trujillo I., Pohlen M., 2008, ApJ, 683, L103 | en_US |
dc.identifier.citedreference | Bland‐Hawthorn J., Vlajić M., Freeman K. C., Draine B. T., 2005, ApJ, 629, 239 | en_US |
dc.identifier.citedreference | Borch A. et al., 2006, A&A, 453, 869 | en_US |
dc.identifier.citedreference | Bournaud F., Elmegreen B. G., Elmegreen D. M., 2007, ApJ, 670, 237 | en_US |
dc.identifier.citedreference | Buitrago F., Trujillo I., Conselice C. J., Bouwens R. J., Dickinson M., Yan H., 2008, ApJ, 687, L61 | en_US |
dc.identifier.citedreference | de Vaucouleurs G., 1959, Handb. Phys., 53, 311 | en_US |
dc.identifier.citedreference | Debattista V. P., Mayer L., Carollo C. M., Moore B., Wadsley J., Quinn T., 2006, ApJ, 645, 209 | en_US |
dc.identifier.citedreference | Elmegreen B. G., Parravano A., 1994, ApJ, 435, L121 | en_US |
dc.identifier.citedreference | Erwin P., Beckman J. E., Pohlen M., 2005, ApJ, 626, L81 | en_US |
dc.identifier.citedreference | Erwin P., Pohlen M., Beckman J. E., 2008, AJ, 135, 20 | en_US |
dc.identifier.citedreference | Ferguson A., Irwin M., Chapman S., Ibata R., Lewis G., Tanvir N., 2007, in de Jong R. S., ed., Island Universes: Structure and Evolution of Disk Galaxies. Springer, Dordrecht, p. 239 | en_US |
dc.identifier.citedreference | Foyle K., Courteau S., Thacker R. J., 2008, MNRAS, 386, 1821 | en_US |
dc.identifier.citedreference | Freeman K. C., 1970, ApJ, 160, 811 | en_US |
dc.identifier.citedreference | Giavalisco M. et al., 2004, ApJ, 600, L93 | en_US |
dc.identifier.citedreference | Gray M. E. et al., 2009, MNRAS, 393, 1275 | en_US |
dc.identifier.citedreference | Gunn J. E., Gott J. R. I., 1972, ApJ, 176, 1 | en_US |
dc.identifier.citedreference | Heiderman A. et al., 2009, ApJ, 705, 1433 | en_US |
dc.identifier.citedreference | Ibata R., Chapman S., Ferguson A. M. N., Lewis G., Irwin M., Tanvir N., 2005, ApJ, 634, 287 | en_US |
dc.identifier.citedreference | Jedrzejewski R. I., 1987, MNRAS, 226, 747 | en_US |
dc.identifier.citedreference | Kennicutt R. C., Jr, 1989, ApJ, 344, 685 | en_US |
dc.identifier.citedreference | Maltby D. T. et al., 2010, MNRAS, 402, 282 | en_US |
dc.identifier.citedreference | Marinova I. et al., 2009, ApJ, 698, 1639 | en_US |
dc.identifier.citedreference | Moore B., Katz N., Lake G., Dressler A., Oemler A., 1996, Nat, 379, 613 | en_US |
dc.identifier.citedreference | Okamoto T., Nagashima M., 2004, in Diaferio A., ed., IAU Colloq. 195, Outskirts of Galaxy Clusters: Intense Life in the Suburbs. Cambridge Univ. Press, Cambridge, p. 534 | en_US |
dc.identifier.citedreference | Patterson F. S., 1940, Harvard College Obser. Bull., 914, 9 | en_US |
dc.identifier.citedreference | Pavlovsky C., Koekemoer A., Mack J., 2006, ACS Data Handbook, Version 5.0. STScI, Baltimore | en_US |
dc.identifier.citedreference | Peng C. Y., Ho L. C., Impey C. D., Rix H.‐W., 2002, AJ, 124, 266 | en_US |
dc.identifier.citedreference | Pérez I., 2004, A&A, 427, L17 | en_US |
dc.identifier.citedreference | Pohlen M., Trujillo I., 2006, A&A, 454, 759 | en_US |
dc.identifier.citedreference | Pohlen M., Dettmar R., Lütticke R., Aronica G., 2002, A&A, 392, 807 | en_US |
dc.identifier.citedreference | Pohlen M., Zaroubi S., Peletier R. F., Dettmar R., 2007, MNRAS, 378, 594 | en_US |
dc.identifier.citedreference | Roškar R., Debattista V. P., Stinson G. S., Quinn T. R., Kaufmann T., Wadsley J., 2008a, ApJ, 675, L65 | en_US |
dc.identifier.citedreference | Roškar R., Debattista V. P., Quinn T. R., Stinson G. S., Wadsley J., 2008b, ApJ, 684, L79 | en_US |
dc.identifier.citedreference | Schaye J., 2004, ApJ, 609, 667 | en_US |
dc.identifier.citedreference | Sérsic J. L., 1968, Atlas de Galaxias Australes. Obser. Astron., Córdoba, Argentina | en_US |
dc.identifier.citedreference | The L. S., White S. D. M., 1986, AJ, 92, 1248 | en_US |
dc.identifier.citedreference | Trujillo I., Pohlen M., 2005, ApJ, 630, L17 | en_US |
dc.identifier.citedreference | van der Kruit P. C., 1979, A&AS, 38, 15 | en_US |
dc.identifier.citedreference | van der Kruit P. C., 2007, A&A, 466, 883 | en_US |
dc.identifier.citedreference | Wolf C., Meisenheimer K., Rix H.‐W., Borch A., Dye S., Kleinheinrich M., 2003, A&A, 401, 73 | en_US |
dc.identifier.citedreference | Wolf C. et al., 2004, A&A, 421, 913 | en_US |
dc.identifier.citedreference | Wolf C., Hildebrandt H., Taylor E. N., Meisenheimer K., 2008, A&A, 492, 933 | en_US |
dc.identifier.citedreference | Wolf C. et al., 2009, MNRAS, 393, 1302 | en_US |
dc.identifier.citedreference | York D. G. et al., 2000, AJ, 120, 1579 | en_US |
dc.identifier.citedreference | Younger J. D., Cox T. J., Seth A. C., Hernquist L., 2007, ApJ, 670, 269 | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.