Wind from a starburst galaxy nucleus

Chevalier, R. A. ; Clegg, A. W.

[s.l.] : Nature Publishing Group
Published 1985
ISSN:
1476-4687
Source:
Nature Archives 1869 - 2009
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- ...
Type of Medium:
Electronic Resource
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
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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