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| Query : 2018PASJ...70...89Y |
2018PASJ...70...89Y - Publ. Astron. Soc. Jap., 70, 89 (2018)
An application of the Ghosh & Lamb model to the accretion-powered X-ray pulsar X Persei.
YATABE F., MAKISHIMA K., MIHARA T., NAKAJIMA M., SUGIZAKI M., KITAMOTO S., YOSHIDA Y. and TAKAGI T.
Journal keyword(s):
Simbad objects: 4
| Number of rows : 4 |
| 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 | V* X Per | HXB | 03 55 23.0777456088 | +31 02 45.039836148 | 6.090 | 6.840 | 6.720 | O9.5III | 1037 | 0 | ||
| 2 | V* CM Tau | Psr | 05 34 31.9474694616 | +22 00 52.153698024 | ~ | 5476 | 0 | |||||
| 3 | GrW 170817 | GWE | 13 09 48.0850 | -23 22 53.343 | ~ | 2683 | 0 | |||||
| 4 | V* KZ TrA | LXB | 16 32 16.79 | -67 27 39.3 | 17.40 | 18.60 | 18.5 | ~ | 626 | 1 |
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