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| Query : 2004A&A...424..979B |
2004A&A...424..979B - Astronomy and Astrophysics, volume 424, 979-992 (2004/9-4)
Cooling of neutron stars. Hadronic model.
BLASCHKE D., GRIGORIAN H. and VOSKRESENSKY D.N.
Abstract (from CDS):
We study the cooling of isolated neutron stars. The main cooling regulators are introduced: equation of state (EoS), thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. The neutrino emissivity includes the main processes. A strong impact of medium effects on the cooling rates is demonstrated. Taking into account medium effects on reaction rates and on nucleon superfluid gaps modern experimental data can be well explained.
Abstract Copyright: ∼
Journal keyword(s): dense matter - equation of state - neutrinos - stars: evolution - stars: neutron - stars: pulsars: general
CDS comments: JC737-3C3J is a misprint for PSR J0737-3039.
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | PSR B1055-52 | Psr | 10 57 59.0450 | -52 26 56.330 | ~ | 725 | 0 | |||||
| 2 | PSR J1915+1606 | Psr | 19 15 27.99999 | +16 06 27.4034 | 22.5 | ~ | 989 | 1 |
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