A 168-s X-Ray Pulsar in the SMC Observed with ASCA
arXiv:astro-ph/0104230 · doi:10.1093/pasj/53.3.L9
Abstract
This paper has been withdrawn because the class file must not be uploaded.
4 pages, 3 figures, to be published in PASJ. Also available at http://www-cr.scphys.kyoto-u.ac.jp/member/jun/job/
References in corpus (4)
- The Discovery of an Outburst and Pulsed X-ray Flux from SMC X-2 from RXTE Observations
- Discovery of the Slowest X-Ray Pulsar in the SMC, AX J0049.5-7323, with ASCA
- Discovery of pulsations from the Be/X-ray binary RX J0101.3-7211 in the SMC by XMM-Newton
- Discovery of a 9-s X-Ray Pulsar, AX J0049-732, in the Small Magellanic Cloud
Cited by in corpus (4)
- Molecular and Atomic Gas in the Large Magellanic Cloud II. Three-dimensional Correlation between CO and HI
- Review of Discrete X-Ray Sources in the Small Magellanic Cloud: Summary of the ASCA Results and Implication on the Recent Star Forming Activity
- Where Are Be/black-hole Binaries?
- Constraining compactness and magnetic field geometry of X-ray pulsars from the statistics of their pulse profiles