1996A&A...315..453T


Query : 1996A&A...315..453T

1996A&A...315..453T - Astronomy and Astrophysics, volume 315453-462 (1996/11-3)

Aspects of mass transfer in X-ray binaries: a model for three classes of binary millisecond pulsars.

TAURIS T.M.

Abstract (from CDS):

The possibility that some close binary systems in their X-ray phase evolve into a second common envelope and spiral-in phase is very important for the formation of short orbital period binary millisecond pulsars. We demonstrate how simple "bifurcation mechanisms" may lead to the existence of three classes of binary millisecond pulsars and a possible gap in the orbital period distribution. Recent discoveries indicate such a gap could exist. Furthermore, we demonstrate that the expected theoretical correlation between orbital periods and white dwarf companion masses does not seem to fit recent observations of wide-orbit (Porb>100days) low-mass binary pulsars.

Abstract Copyright: ∼

Journal keyword(s): binaries: general - stars: evolution - stars: neutron - pulsars: general

Simbad objects: 34

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Number of rows : 34
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J0034-05 Psr 00 34 21.8281 -05 34 36.620           ~ 201 0
2 LAWD 10 WD* 01 37 59.3936818351 -04 59 44.668541360   13.20 12.83 12.8   DA+D1 191 0
3 PSR J0218+42 Psr 02 18 06.3604 +42 32 17.365           ~ 365 2
4 PSR J0437-47 Psr 04 37 15.7994581776 -47 15 08.544351636           DC 1032 0
5 PSR B0613-02.0 Psr 06 13 43.977070 -02 00 47.34294           ~ 319 1
6 PSR J0621+10 Psr 06 21 22.11108 +10 02 38.7410           ~ 128 1
7 PSR B0655+64 Psr 07 00 37.802 +64 18 11.20           ~ 250 1
8 PSR J0751+1807 Psr 07 51 09.1539 +18 07 38.335           ~ 316 1
9 PSR J0823+0159 Psr 08 23 09.78731 +01 59 12.6003           DA 244 0
10 PSR J1012+5307 Psr 10 12 33.4345449600 +53 07 02.548542576     19.5     DA 419 1
11 PSR J1022+10 Psr 10 22 57.990 +10 01 52.92           ~ 279 2
12 PSR J1045-45 Psr 10 45 50.179671 -45 09 54.05686           ~ 154 1
13 PSR B1257+12 Psr 13 00 03.1075 +12 40 55.155           ~ 546 1
14 PSR J1455-3300 Psr 14 55 47.976991 -33 30 46.40280           ~ 165 1
15 PSR J1604-72 Psr 16 03 35.670781 -72 02 32.82328           ~ 142 0
16 PSR J1640+2224 Psr 16 40 16.744850 +22 24 08.84119           ~ 210 0
17 PSR J1643-1224 Psr 16 43 38.16612 -12 24 58.6334           ~ 260 2
18 PSR J1713+0747 Psr 17 13 49.5367813 +07 47 37.450240           ~ 530 1
19 PSR B1718-19 Psr 17 21 01.48 -19 36 51.0           ~ 97 1
20 PSR B1800-27 Psr 18 03 31.692 -27 12 06.00           ~ 57 0
21 PSR J1804-27 Psr 18 04 21.13307 -27 17 31.3370           ~ 87 1
22 PSR B1831-00 Psr 18 34 17.25 -00 10 53.3           DA 101 0
23 PSR B1855+09 Psr 18 57 36.390620 +09 43 17.20712           DA 569 1
24 PSR J1911-11 Psr 19 11 49.2927 -11 14 22.330           ~ 87 1
25 PSR J1915+1606 Psr 19 15 27.99999 +16 06 27.4034     22.5     ~ 1032 1
26 PSR B1953+29 Psr 19 55 27.8680959374 +29 08 43.499227152           ~ 303 1
27 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3
28 PSR J2019+24 Psr 20 19 31.94900 +24 25 15.3038           ~ 145 1
29 PSR J2033+1736 Psr 20 33 16.9140266736 +17 37 48.047177388   11.59 10.50     ~ 76 0
30 V* LY Aqr Psr 20 51 07.52058 -08 27 37.6100           ~ 236 2
31 PSR J2129-5718 Psr 21 29 22.781548 -57 21 14.33356           ~ 122 1
32 PSR B2145-07.8 Psr 21 45 50.45590 -07 50 18.5900           ~ 336 0
33 PSR J2229+26 Psr 22 29 50.883815 +26 43 57.61393           ~ 121 1
34 PSR J2317+1439 Psr 23 17 09.235606 +14 39 31.29559           ~ 211 1

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