Details on Acronym: [FRP2003] | |
| [FRP2003] | (Franciosini+Randich+Pallavicini, 2003) |
| Write: | <<[FRP2003] JHHMMSS.ss+DDMMSS.s>> |
| N: | 24 |
| Object: | (X) (SIMBAD class: X = X-ray Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | XMM-Newton observations of the Hyades cluster. N=24 X-ray sources with at least an optical counterpart which is a cluster non-member or has no membership information. |
| Ref: | =2003A&A...405..551F |
| by | FRANCIOSINI E. , RANDICH S., PALLAVICINI R. |
| Astron. Astrophys., 405, 551-561 (2003) | |
| Is Praesepe really different from the coeval Hyades cluster? The XMM-Newton view. | |
| o | In table 3, GSC2 N231230081115 is a misprint for N23123008115. KW = Cl* NGC 2632 KW, JS = Cl* NGC 2632 JS, HSHJ = Cl* NGC 2632 HSHJ, WRS = Cl* NGC 2632 WRS in SIMBAD |
| o | Table 3: <[FRP2003] JHHMMSS.ss+DDMMSS.s> N=24. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |