An analysis of optical periods in individual Small Magellanic Cloud Be/X-ray pulsars-Reference-Cited by-同舟云学术

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An analysis of optical periods in individual Small Magellanic Cloud Be/X-ray pulsars

Published:2013-02-27 Issue:1 Volume:431 Page:252-278
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Schmidtke P. C.,Cowley A. P.,Udalski A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/431/1/252/18239185/stt159.pdf

Reference141 articles.

1. The MACHO Project Large Magellanic Cloud Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo

2. Short-period line profile and light variations in the Be star Eridani

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1. Population synthesis of Be X-ray binaries: metallicity dependence of total X-ray outputs;Monthly Notices of the Royal Astronomical Society;2023-11-13

2. Long-term Variability of Non-radial Pulsations in SXP 4.78;Research Notes of the AAS;2022-08-18

3. Stability of Nonradial Pulsations in the Be Star [MA93]1506;Research Notes of the AAS;2021-11-16

4. SRG/eROSITA discovery of 164s pulsations from the SMC Be/X-ray binary XMMU J010429.4-723136;Astronomy & Astrophysics;2021-11-01

5. XMMU J050722.1−684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507−6847;Monthly Notices of the Royal Astronomical Society;2021-03-18

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