| LW2020] (Cheng+Li+Wang+, 2020) | Details on Acronym: [CLW2020] | |
| [CLW2020] | ||
| Write: | <<[CLW2020] NNN>> | |
| N: | 300 | |
| Object: | (X) (SIMBAD class: X = X-ray Source) | |
| Note: | N=300 X-ray sources in ω Cen. Use of archival Chandra data. See also [CLF2019], [CLL2019], [CML2020]. | |
| in source: | NGC 5139 = ome Cen | |
| Ref: | =2020ApJ...904..198C | |
| by | CHENG Z. , LI Z., WANG W., LI X., XU X. | |
| Astrophys. J., 904, 198-198 (2020) | ||
| Exploring the mass segregation effect of X-ray sources in globular clusters. IV. Evidence of black hole burning in ω Centauri. | ||
| o | Table 1: <[CLW2020] NNN> (Nos 1-300). | |
| Origin | of the Acronym: D = Assigned by the Dictionary of Acronyms | |