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Conference Paper: A Deep Tech Pan Survey of Dwarf Spheroidal Galaxies in Virgo
Title | A Deep Tech Pan Survey of Dwarf Spheroidal Galaxies in Virgo |
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Authors | |
Editors | Editor(s):Morganti, R |
Issue Date | 1999 |
Citation | Looking Deep in the Southern Sky: Proceedings of the ESO/Australia Workshop, Sydney, Australia, 10–12 December 1997, p. 83-88 How to Cite? |
Abstract | We have made a very deep photographic R band survey of a region of the Virgo Cluster by utilising digital stacking of scans of Tech Pan films taken on the U.K. Schmidt Telescope. The objects we detect have the same physical sizes and surface brightnesses as Local Group dwarf spheroidal galaxies. The luminosity function of these extremely low luminosity galaxies (down to M R ≃ −11 or about 5 × 10−5 L *) is very steep, with a power law slope α ≃ −2, supporting previous observational evidence at somewhat higher luminosities in other clusters. |
Persistent Identifier | http://hdl.handle.net/10722/211273 |
ISBN | |
ISSN | |
Series/Report no. | ESO Astrophysics Symposia |
DC Field | Value | Language |
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dc.contributor.author | Parker, QA | - |
dc.contributor.author | Phillipps, S | - |
dc.contributor.author | Couch, WJ | - |
dc.contributor.editor | Morganti, R | - |
dc.date.accessioned | 2015-07-08T03:24:01Z | - |
dc.date.available | 2015-07-08T03:24:01Z | - |
dc.date.issued | 1999 | - |
dc.identifier.citation | Looking Deep in the Southern Sky: Proceedings of the ESO/Australia Workshop, Sydney, Australia, 10–12 December 1997, p. 83-88 | - |
dc.identifier.isbn | 9783662221198 | - |
dc.identifier.issn | 1431-2433 | - |
dc.identifier.uri | http://hdl.handle.net/10722/211273 | - |
dc.description.abstract | We have made a very deep photographic R band survey of a region of the Virgo Cluster by utilising digital stacking of scans of Tech Pan films taken on the U.K. Schmidt Telescope. The objects we detect have the same physical sizes and surface brightnesses as Local Group dwarf spheroidal galaxies. The luminosity function of these extremely low luminosity galaxies (down to M R ≃ −11 or about 5 × 10−5 L *) is very steep, with a power law slope α ≃ −2, supporting previous observational evidence at somewhat higher luminosities in other clusters. | - |
dc.language | eng | - |
dc.relation.ispartof | Looking Deep in the Southern Sky | - |
dc.relation.ispartofseries | ESO Astrophysics Symposia | - |
dc.title | A Deep Tech Pan Survey of Dwarf Spheroidal Galaxies in Virgo | - |
dc.type | Conference_Paper | - |
dc.identifier.email | Parker, QA: quentinp@hku.hk | - |
dc.identifier.authority | Parker, QA=rp02017 | - |
dc.identifier.doi | 10.1007/978-3-540-49460-7_16 | - |
dc.identifier.spage | 88 | - |
dc.identifier.epage | 83 | - |
dc.identifier.eissn | 1611-6143 | - |
dc.identifier.issnl | 1431-2433 | - |