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Details on Acronym: eps Cha
eps Cha (eps Cha Group) ***** Avoid the usage of eps Cha, prefer [FLG2003] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: [FLG2003]
[FLG2003] (Feigelson+Lawson+Garmire, 2003)= (eps Cha) Write:<<[FLG2003] eps Cha NN>>
<<[FLG2003] JHHMMSS.s+DDMMSS.s>> N: 21+10+19 Object:*inCl + (X) (SIMBAD class: Unknown = Object of Unknown Nature) Stat:is completely incorporated in Simbad Note:Chandra observations of the eps Cha Group of stars.
N=21 stars are members of the group. N=10 new X-ray selected members of the 'OSCA' association (Oph-Sco-Cen Assoc.). in source:NAME EPS CHA GROUP Ref:=2003ApJ...599.1207F byFEIGELSON E.D. , LAWSON W.A., GARMIRE G.P. Astrophys. J., 599, 1207-1222 (2003) The ε Chamaeleontis young stellar group and the characterization of sparse stellar clusters. o(Erratum) erratum vol.649, p. 1184 (2006) oTable 3: <[FLG2003] eps Cha N> (Nos 1-9). Table 4: <[FLG2003] JHHMMSS.s+DDMMSS.s> N=10. Ref:=2004ApJ...616.1033L byLUHMAN K.L. Astrophys. J., 616, 1033-1041 (2004) A survey for low-mass stars and brown dwarfs in the η Chamaeleontis and ε Chamaeleontis young associations. oTable 3: <[FLG2003] eps Cha NN> (Nos 10-12) added. Ref:=2008ApJ...675.1375L byLUHMAN K.L. , ALLEN L.E., ALLEN P.R., GUTERMUTH R.A., HARTMANN L., MAMAJEK E.E., MEGEATH S.T., MYERS P.C., FAZIO G.G. Astrophys. J., 675, 1375-1406 (2008) The disk population of the Chamaeleon I star-forming region. oTables 4-7: <[L2007b] Cha JHHMMSSss+DDMMSSs> N=17 added. Table 11: <[FLG2003] eps Cha NN> (Nos 13-21) added. Ref:=2013MNRAS.435.1325M byMURPHY S.J. , LAWSON W.A., BESSELL M.S. Mon. Not. R. Astron. Soc., 435, 1325-1349 (2013) Re-examining the membership and origin of the ε Cha association. oTable 7: <[FLG2003] eps Cha NN> (Nos 22-40) added. =E=Catalogue in electronic form as J/ApJ/675/1375 Originof the Acronym: S = Created by Simbad, the CDS Database
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