Wind from a starburst galaxy nucleus
| 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
|
| Notes: |
[Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ...
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798293100539412480 |
|---|---|
| autor | Chevalier, R. A. Clegg, A. W. |
| book_url | http://dx.doi.org/10.1038/317044a0 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLZ235411892 |
| insertion_date | 1911-02-25 |
| issn | 1476-4687 |
| journal_name | Nature |
| materialart | 1 |
| notes | [Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ... |
| package_name | Nature Publishing Group |
| publikationsjahr_anzeige | 1985 |
| publikationsjahr_facette | 1985 |
| publikationsjahr_intervall | 8014:1985-1989 |
| publikationsjahr_sort | 1985 |
| publikationsort | [s.l.] |
| publisher | Nature Publishing Group |
| reference | 317 (1985), S. 44-45 |
| search_space | articles |
| shingle_author_1 | Chevalier, R. A. Clegg, A. W. |
| shingle_author_2 | Chevalier, R. A. Clegg, A. W. |
| shingle_author_3 | Chevalier, R. A. Clegg, A. W. |
| shingle_author_4 | Chevalier, R. A. Clegg, A. W. |
| shingle_catch_all_1 | Chevalier, R. A. Clegg, A. W. Wind from a starburst galaxy nucleus Nature Publishing Group [Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ... 1476-4687 14764687 |
| shingle_catch_all_2 | Chevalier, R. A. Clegg, A. W. Wind from a starburst galaxy nucleus Nature Publishing Group [Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ... 1476-4687 14764687 |
| shingle_catch_all_3 | Chevalier, R. A. Clegg, A. W. Wind from a starburst galaxy nucleus Nature Publishing Group [Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ... 1476-4687 14764687 |
| shingle_catch_all_4 | Chevalier, R. A. Clegg, A. W. Wind from a starburst galaxy nucleus Nature Publishing Group [Auszug] We assume that the wind is spherically symmetrical and that gravitational forces are negligible. The total mass and energy input are M and ‰ respectively. The equations for the flow are3: du dP - =---qu dt dr (1) (2) where for r 〈 R, q = M/ V9 Q = ‰/ V, V = | tt3, and for r〉 R, q- ... 1476-4687 14764687 |
| shingle_title_1 | Wind from a starburst galaxy nucleus |
| shingle_title_2 | Wind from a starburst galaxy nucleus |
| shingle_title_3 | Wind from a starburst galaxy nucleus |
| shingle_title_4 | Wind from a starburst galaxy nucleus |
| sigel_instance_filter | dkfz geomar wilbert ipn albert |
| source_archive | Nature Archives 1869 - 2009 |
| timestamp | 2024-05-06T08:59:03.227Z |
| titel | Wind from a starburst galaxy nucleus |
| titel_suche | Wind from a starburst galaxy nucleus |
| topic | W V WW-YZ TA-TD U |
| uid | nat_lic_papers_NLZ235411892 |