Details on Acronym: [PFR2002] | |
| [PFR2002] | (Patnaude+Fesen+Raymond+, 2002) |
| Write: | <<[PFR2002] ISM Cloud>> <<[PFR2002] N>> <<[PFR2002] AN>> |
| N: | 1+6+6+4+3+4 |
| Object: | Region (SIMBAD class: Region = Region defined in the Sky) |
| Note: | ROSAT and ground-based observations of the Cygnus Loop. N=1 Interstellar medium (ISM) cloud, N=6 X-ray regions (Nos 1-6), N=6 Balmer-dominated filaments (Nos B1-B6), N=4 OIII bright regions (Nos O1-O4), N=3 radiative filaments (Nos R1-R3), N=4 sulfur bright regions (Nos S1-S4). |
| in source: | X Cyg X-5 |
| Ref: | =2002AJ....124.2118P |
| by | PATNAUDE D.J. , FESEN R.A., RAYMOND J.C., LEVENSON N.A., GRAHAM J.R., WALLACE D.J. |
| Astron. J., 124, 2118-2134 (2002) | |
| An isolated, recently shocked ISM cloud in the Cygnus Loop supernova remnant. | |
| o | Figs: <[PFR2002] ISM Cloud> N=1. Fig.15, Table 2: <[PFR2002] N> (Nos 1-6). Fig.7: <[PFR2002] AN> (Nos B1-B6). Fig.10: <[PFR2002] AN> (Nos O1-O4, R1-R3, S1-S4). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |