| Autor: |
W.T.S. Deich, S.R. Kulkarni |
| Rok vydání: |
1996 |
| Předmět: |
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| Zdroj: |
Symposium - International Astronomical Union. 165:279-285 |
| ISSN: |
0074-1809 |
| DOI: |
10.1017/s0074180900055741 |
| Popis: |
Several years of timing the pulsar in the binary neutron star system M15C have yielded the masses of both stars: the total mass is MT = 2.7121(6) M⊙; the companion mass is mc = 1.36(4) M⊙; and the pulsar mass is mp = 1.35(4) M⊙. We argue that this system is not likely to have formed through accretion-induced collapse (AIC), and that the standard model also has problems in explaining the formation. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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