Details on Acronym: [BSN97] | |
| [BSN97] | (Beekman+Shahbaz+Naylor+, 1997) |
| Write: | <<[BSN97] Comparison star>> <<[BSN97] Standard N>> |
| N: | 1+2 |
| Object: | * (SIMBAD class: Star) |
| Stat: | is completely incorporated in Simbad |
| Note: | UKIRT observations. Comparison and standard stars in the field of GRO J0422+32. See also [CI95]. |
| Ref: | =1997MNRAS.290..303B |
| by | BEEKMAN G. , SHAHBAZ T., NAYLOR T., CHARLES P.A., WAGNER R.M., MARTINI P. |
| Mon. Not. R. Astron. Soc., 290, 303-312 (1997) | |
| The mass of the black hole in the low-inclination LMXB transient system GRO J0422 + 32 (=Nova Persei 1992). | |
| o | [BSN97] Standard 2 is not the same star as [CI95] 2. |
| o | Table 2: <[BSN97] Comparison star> N=1, <[BSN97] Standard N> (Nos 1-2). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |