Details on Acronym: YLW
YLW (Young+Lada+Wilking) Write:<<YLW NNA>> N: 77 Object:(IR) (SIMBAD class: Infrared = Infra-Red Source) Stat:is completely incorporated in Simbad in source:NAME rho Oph Cloud Ref:=1986ApJ...304L..45Y byYOUNG E.T. , LADA C.J., WILKING B.A. Astrophys. J., 304, 45-49 (1986) High-resolution IRAS observations of the ρ Ophiuchi cloud core. oTable 1: <YLW NN> (Nos 1-18), <YLW NNA> N=31. Ref:=1989ApJ...340..823W byWILKING B.A. , LADA C.J., YOUNG E.T. Astrophys. J., 340, 823-852 (1989) IRAS observations of the ρ Ophiuchi infrared cluster : spectral energy distributions and luminosity function. oTable 1: <WLY 1-NN> (Nos 1-64), Table 2: <WLY 2-NNa> (Nos 1-58, 32b). Table 4: <YLW NNN> (Nos 1-60). Ref:=1995ApJ...438..813S bySTROM K.M. , KEPNER J., STROM S.E. Astrophys. J., 438, 813-829 (1995) The evolutionary status of the stellar population in the ρ Ophiuchi cloud core. oNot in SIMBAD: DoAr 24E oTables 1, 3: <[SKS95] HHMMSS.s-DDMMSS> N=119, Table 4: <[SKS95] aN> N=5. Table 1: <YLW NNA> (No. 46A) Ref:=1998MNRAS.299..699L byLUCAS P.W. , ROCHE P.F. Mon. Not. R. Astron. Soc., 299, 699-722 (1998) Imaging polarimetry of class I young stellar objects. oTable 5: <YLW NNA> (Nos 16C-16D). Originof the Acronym: L = Found in the literature
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