Details on Acronym: [VZK2001] | |
[VZK2001] | (Van Loon+Zijlstra+Kaper+, 2001) |
Write: | <<[VZK2001] HS 327W>> <<[VZK2001] A>> <<[VZK2001] Carbon>> <<[VZK2001] Red>> |
N: | 2+3+1+1 |
Object: | Cluster of * + * (SIMBAD class: Star) |
Stat: | is completely incorporated in Simbad |
Note: | Fig.2: [HS66] 327 is composed of 2 distinct stellar clusters: HS 327W and HS 327E. Tables 1, 2: N=3 brightest stars (Nos A-C), N=1 Carbon star, and N=1 Red star. |
in source: | Magellanic Clouds:LMC:[HS66] 327 = [HS66] 327 |
Ref: | =2001A&A...368..239V |
by | VAN LOON J.T. , ZIJLSTRA A.A., KAPER L., GILMORE G.F., LOUP C., BLOMMAERT J.A.D.L. |
Astron. Astrophys., 368, 239-249 (2001) | |
The peculiar cluster HS 327 in the Large Magellanic Cloud: can OH/IR stars and carbon stars be twins? | |
o | Standard star S 121-E = GSPC S121-E |
o | Text: <[VZK2001] HS 327W> (Nos E, W). Tables 1, 2: <[VZK2001] A> (Nos A-C), <[VZK2001] Carbon> N=1, <[VZK2001] Red> N=1. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |