Details on Acronym: [DK2003] | |
[DK2003] | (Di Stefano+Kong, 2003) |
Write: | <<[DK2003] M101-NNN>> <<[DK2003] M51-NN>> <<[DK2003] M83-NNN>> |
Object: | (X) (SIMBAD class: X = X-ray Source) |
Stat: | is completely incorporated in Simbad |
Note: | Chandra data are used to identify luminous candidate supersoft X-ray sources in 3 external galaxies. See also [PSM2001], [SW2002b], [SW2003]. |
in source: | M 101 = NGC 5457 |
in source: | M 51 = NGC 5194 |
in source: | M 83 = NGC 5236 |
Ref: | =2003ApJ...592..884D |
by | DI STEFANO R. , KONG A.K.H. |
Astrophys. J., 592, 884-899 (2003) | |
Luminous supersoft X-ray sources in external galaxies. | |
o | In the abstract NGC 4967 is a misprint for NGC 4697. Table 3: Objects in NGC 4697 are [SIB2001] in SIMBAD. |
o | Table 3: <[DK2003] M101-NNN> N=16 among (Nos 15-104), <[DK2003] M51-NN> N=4 among (Nos 12-58), <[DK2003] M83-NNN> N=10 among (Nos 20-128). |
Ref: | =2004ApJ...609..710D |
by | DI STEFANO R. , KONG A.K.H. |
Astrophys. J., 609, 710-727 (2004) | |
The discovery of quasi-soft and supersoft sources in external galaxies. | |
o | In Abstract : NGC 4967 is a misprint for NGC 4697. Table 4: Sources in NGC 4697 are [SIB2001] in SIMBAD. |
o | Table 1: <[DK2003] M101-NNN> N=37 added among (Nos 2-116). Table 2: <[DK2003] M83-NNN> N=44 added among (Nos 1-127). Table 3: <[DK2003] M51-NN> N=20 added among (Nos 5-70). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |