2003A&A...407..259Y


Query : 2003A&A...407..259Y

2003A&A...407..259Y - Astronomy and Astrophysics, volume 407, 259-263 (2003/8-3)

What we can learn from observations of cooling neutron stars.

YAKOVLEV D.G. and HAENSEL P.

Abstract (from CDS):

A generic toy model of a cooling neutron star (NS) is used to analyze cooling of NSs with nucleon and exotic compositions of the cores. The model contains the parameters which specify the levels of slow and fast neutrino emission as well as the lower and upper densities of the layer where the slow emission transforms into the fast one. The prospects to constrain these parameters from the present and future observations of isolated middle-aged NSs are discussed.

Abstract Copyright:

Journal keyword(s): stars: neutron - dense matter

CDS comments: 1E 1207-52 = 1E 1207.3-5210.

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 TYC 4018-3227-1 * 00 02 55.7100664872 +62 46 17.662572696   12.49 11.67     ~ 39 1
2 NAME Geminga Psr 06 33 54.153 +17 46 12.91           ~ 1177 0
3 PSR B0656+14 Psr 06 59 48.1960 +14 14 19.400   24.85 24.90     ~ 830 1
4 PSR J0821-4300 Psr 08 21 58.2 -43 00 22           ~ 122 2
5 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2245 1
6 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 707 0
7 SNR G295.5+09.7 SNR 12 09 40 -52 25.0           ~ 279 1
8 RX J1856.6-3754 Psr 18 56 35.11 -37 54 30.5     25.7     ~ 423 0

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2023.03.30-07:24:28

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