Details on Acronym: CH | |
CH | (Carbon, Hydrogen) |
***** | Avoid the usage of CH, prefer [HC88] |
Origin | of the Acronym: L = Found in the literature |
Details on Acronym: HC | |
HC | (Hartwick+Cowley) |
***** | Avoid the usage of HC, prefer [HC88] |
Origin | of the Acronym: L = Found in the literature |
Details on Acronym: [HC88] | |
[HC88] | (Hartwick+Cowley, 1988)= (CH) = (HC) = (LMC CH) |
Write: | <<[HC88] NNN>> |
N: | 53 |
Object: | CH * (SIMBAD class: Star) |
Note: | N=53 among (Nos 1-222) |
in source: | Magellanic Clouds:LMC = LMC |
Ref: | =1988ApJ...334..135H |
by | HARTWICK F.D.A. , COWLEY A.P. |
Astrophys. J., 334, 135-143 (1988) | |
The kinematics of an old stellar population in the Large Magellanic Cloud : the CH stars. | |
o | <[HC88] NNN> N=53 among (Nos 1-222) |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: LMC CH | |
LMC CH | (LMC, CH) |
***** | Avoid the usage of LMC CH, prefer [HC88] |
Origin | of the Acronym: A = Assigned by the author(s) |