2008A&A...483..249M


C.D.S. - SIMBAD4 rel 1.7 - 2020.04.08CEST14:18:17

2008A&A...483..249M - Astronomy and Astrophysics, volume 483, 249-251 (2008/5-3)

Swift observations of the X-ray pulsar SAX J1324-6200.

MEREGHETTI S., ROMANO P. and SIDOLI L.

Abstract (from CDS):

We present recent observations of the X-ray pulsar SAX J1324-6200 obtained in December 2007 with the Swift satellite, significantly improving the source localization over previous data and providing a new measurement of the spin period P=172.84s. A single object that is consistent in colors with a highly reddened early type star is visible in the X-ray error box. The period is significantly longer than what was obtained in 1997, indicating that SAX J1324-6200 has been spinning down at an average rate of ∼6x10–9s/s. We discuss the possible nature of the source, showing that it most likely belongs to the class of low-luminosity, persistent Be/neutron star binaries.

Abstract Copyright:

Journal keyword(s): X-rays: binaries

Status at CDS:  

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 - 2020
#notes
1 V* X Per HXB 03 55 23.0778791365 +31 02 45.045745259 6.090 6.840 6.720     O9.5III 899 0
2 NAME Car Arm PoG 10 00 -60.0           ~ 373 1
3 NAME Crux Arm PoG 12 30 -60.0           ~ 81 0
4 SAX J1324.4-6200 HXB 13 24 26.70 -62 01 19.5           Be? 20 0
5 4U 1323-62 LXB 13 26 36.31 -62 08 09.9           ~ 162 0
6 V* KZ TrA LXB 16 32 16.79 -67 27 39.3 17.40 18.60 18.5     ~ 522 1
7 V* V2116 Oph Sy* 17 32 02.1544831482 -24 44 44.125962969   20.78 18.4     M6IIIe 644 1
8 4U 1907+09 HXB 19 09 37.9 +09 49 49   19.41 16.35 14.40 12.53 O8.5Iab 307 1

    Equat.    Gal    SGal    Ecl

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2020.04.08-14:18:17

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