Details on Acronym: [KKM89] | |
| [KKM89] | (Koyama+Kondo+Makino+, 1989) |
| Write: | <<[KKM89] N>> |
| N: | 4 |
| Object: | (X) (SIMBAD class: X = X-ray Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | N=4 X-ray transient sources, discovered with the Ginga satellite. See also [KKK90]. |
| Ref: | =1989PASJ...41..483K |
| by | KOYAMA K. , KONDO H., MAKINO F., NAGASE F., TAKANO S., TAWARA Y., TURNER M.J.L., WARWICK R.S. |
| Publ. Astron. Soc. Jap., 41, 483-490 (1989) | |
| Are there many Be star binary X-ray pulsars in the galactic ridge ? | |
| o | Table 2: <[KKM89] N> (Nos 1-4). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |