A runaway instability in thick accretion disks?
| ISSN: |
1476-4687
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|---|---|
| Source: |
Nature Archives 1869 - 2009
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| Topics: |
Biology
Chemistry and Pharmacology
Medicine
Natural Sciences in General
Physics
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| Notes: |
[Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ...
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798293104546021376 |
|---|---|
| autor | Wilson, D. B. |
| book_url | http://dx.doi.org/10.1038/312620a0 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLZ235437425 |
| insertion_date | 1911-02-25 |
| issn | 1476-4687 |
| journal_name | Nature |
| materialart | 1 |
| notes | [Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ... |
| package_name | Nature Publishing Group |
| publikationsjahr_anzeige | 1984 |
| publikationsjahr_facette | 1984 |
| publikationsjahr_intervall | 8019:1980-1984 |
| publikationsjahr_sort | 1984 |
| publikationsort | [s.l.] |
| publisher | Nature Publishing Group |
| reference | 312 (1984), S. 620-621 |
| search_space | articles |
| shingle_author_1 | Wilson, D. B. |
| shingle_author_2 | Wilson, D. B. |
| shingle_author_3 | Wilson, D. B. |
| shingle_author_4 | Wilson, D. B. |
| shingle_catch_all_1 | Wilson, D. B. A runaway instability in thick accretion disks? Nature Publishing Group [Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ... 1476-4687 14764687 |
| shingle_catch_all_2 | Wilson, D. B. A runaway instability in thick accretion disks? Nature Publishing Group [Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ... 1476-4687 14764687 |
| shingle_catch_all_3 | Wilson, D. B. A runaway instability in thick accretion disks? Nature Publishing Group [Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ... 1476-4687 14764687 |
| shingle_catch_all_4 | Wilson, D. B. A runaway instability in thick accretion disks? Nature Publishing Group [Auszug] The construction of disk models in the standard approach, due to the school of Abramowicz, is straightforward23. For an axisymmetric stationary space-time, the metric has the form4 ds2= -e2v at2+r2B2 sin2 ? e2?(?f - ? at)2 + e2/A(dr2+r2dlt;92) (1) where zgt;, , ? and B are functions of polar ... 1476-4687 14764687 |
| shingle_title_1 | A runaway instability in thick accretion disks? |
| shingle_title_2 | A runaway instability in thick accretion disks? |
| shingle_title_3 | A runaway instability in thick accretion disks? |
| shingle_title_4 | A runaway instability in thick accretion disks? |
| sigel_instance_filter | dkfz geomar wilbert ipn albert |
| source_archive | Nature Archives 1869 - 2009 |
| timestamp | 2024-05-06T08:59:06.536Z |
| titel | A runaway instability in thick accretion disks? |
| titel_suche | A runaway instability in thick accretion disks? |
| topic | W V WW-YZ TA-TD U |
| uid | nat_lic_papers_NLZ235437425 |