Details on Acronym: CK | |
CK | (Cohen+Kuhi) |
***** | Avoid the usage of CK, prefer CoKu |
Origin | of the Acronym: L = Found in the literature |
Details on Acronym: CoKu | |
CoKu | (Cohen+Kuhi)= (CK) |
Write: | <<CoKu {UZ Tau} {f|p}>> <<CoKu DO Tau East>> <<CoKu {LkHA 346} W{f|p}>> <<CoKu AA CCC GN>> <<CoKu LkHA NNN GN>> <<CoKu Haro 2-249 GN>> <<CoKu Ser GN>> <<CoKu NGC NNNN Star N>> <<CoKu Tau-Aur Star N>> <<CoKu Mon R2 Star N>> <<CoKu Small Group Star N>> <<CoKu NGC 7000/IC 5070 IRS N>> <<CoKu AA CCC c>> <<CoKu V447 Ori c>> <<CoKu Haro N-NNN c>> <<CoKu LkHA NNN c>> <<CoKu AS NNN c>> <<CoKu Parenago NNNN c>> <<CoKu Ser G1 c>> <<CoKu SR 24 c>> <<CoKu MWC 1080 c>> |
N: | 90 |
Object: | * (SIMBAD class: Star) |
Stat: | is completely incorporated in Simbad |
Note: | In the format the letter 'G' stands for 'small Group of stars', around another star. At the end of the format the letter 'a' stands for 'f' (forwarding) or 'p' (precessing) At the end of the format the letter 'c' stands for 'companion' of another star. The formats are often found ending with '/GN', '/N', '/IRSN', or '/c'. |
Ref: | =1979ApJS...41..743C |
by | COHEN M. , KUHI L.V. |
Astrophys. J., Suppl. Ser., 41, 743-843 (1979) | |
Observational studies of pre-main-sequence evolution. | |
o | <CoKu UZ Tau a>, <CoKu DO Tau East>, <CoKu LkHA 346 Na>, <CoKu AA CCC GN>, <CoKu LkHA NNN GN>, <CoKu Haro 2-249 GN>, <CoKu Ser GN> N=39. <CoKu NGC NNNN Star N>, <CoKu Tau-Aur Star N>, <CoKu Mon R2 Star N>, <CoKu Small Group N>, <CoKu NGC 7000/IC 5070 IRS N>, <CoKu AA CCC c>, <CoKu V447 Ori c>, <CoKu Haro N-NNN c>, <CoKu LkHA NNN c> <CoKu AS NNN c>, <CoKu Parenago NNNN c>, <CoKu Ser G1 c>, <CoKu MWC 1080 c> N=81 |
Origin | of the Acronym: L = Found in the literature |