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Luminosity versus Phase-Space-Density Relation of Galaxies Revisited
http://hdl.handle.net/10091/10116
http://hdl.handle.net/10091/101163290ad89-3e14-4324-a191-e2fa1484d045
| 名前 / ファイル | ライセンス | アクション |
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ApJ_531_665.pdf (138.3 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||||||||
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| 公開日 | 2010-06-03 | |||||||||||
| タイトル | ||||||||||||
| タイトル | Luminosity versus Phase-Space-Density Relation of Galaxies Revisited | |||||||||||
| 言語 | ||||||||||||
| 言語 | eng | |||||||||||
| DOI | ||||||||||||
| 関連識別子 | https://doi.org/10.1086/308498 | |||||||||||
| 関連名称 | 10.1086/308498 | |||||||||||
| キーワード | ||||||||||||
| 主題 | galaxies: clusters: general, galaxies: kinematics and dynamics, galaxies: photometry, galaxies: structure | |||||||||||
| 資源タイプ | ||||||||||||
| 資源 | http://purl.org/coar/resource_type/c_6501 | |||||||||||
| タイプ | journal article | |||||||||||
| 著者 |
Kodaira, K
× Kodaira, K
× Kashikawa, N
× Misawa, T
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| 信州大学研究者総覧へのリンク | ||||||||||||
| 氏名 | Misawa, T | |||||||||||
| URL | http://soar-rd.shinshu-u.ac.jp/profile/ja.ypchuUkV.html | |||||||||||
| 出版者 | ||||||||||||
| 出版者 | The American Astronomical Society | |||||||||||
| 引用 | ||||||||||||
| 内容記述 | The Astrophysical Journal. 531:665-675 (2000) | |||||||||||
| 書誌情報 |
The Astrophysical journal 巻 531, 号 2, p. 665-675, 発行日 2000-03-10 |
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| 抄録 | ||||||||||||
| 内容記述 | We reexamined the correlation between the B-T magnitude and the phase-space-density parameter w = (D-2(25) v(o))(-1) of galaxies for the Virgo, the Coma, the Fornax, and the Perseus clusters in an effort to better understand the physical underpinning of the fundamental plane. A tight correlation (B-T = a log w + b) common to different morphological types of galaxies (E, S0, S) was found for the Virgo and the Coma clusters, with a = 1.87 +/- 0.10 and 1.33 +/- 0.11, respectively. An investigation using only E galaxies was made for the four clusters. The results indicated that the empirical linear relation might be common among the Coma, the Fornax, and the Perseus clusters, with the Virgo Cluster showing deviation. This relation, which is another way to project the fundamental plane, has an expression insensitive to the morphology and may be suitable for treating galaxies of different morphological types collectively. | |||||||||||
| 資源タイプ（コンテンツの種類） | ||||||||||||
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| 収録物識別子タイプ | ISSN | |||||||||||
| 収録物識別子 | 0004-637X | |||||||||||
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| 収録物識別子タイプ | NCID | |||||||||||
| 収録物識別子 | AA00553253 | |||||||||||
| 出版タイプ | ||||||||||||
| 出版タイプ | VoR | |||||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||||
| WoS | ||||||||||||
| URL | http://gateway.isiknowledge.com/gateway/Gateway.cgi?&GWVersion=2&SrcAuth=ShinshuUniv&SrcApp=ShinshuUniv&DestLinkType=FullRecord&DestApp=WOS&KeyUT=000086201300007 | |||||||||||
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Kodaira, K, Kashikawa, N, Misawa, T, 2000, Luminosity versus Phase-Space-Density Relation of Galaxies Revisited: The American Astronomical Society, 665–675 p.
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