Details on Acronym: [HRF2005]
[HRF2005] (Hatchell+Richer Fuller+, 2005) Write:<<[HRF2005] NN>> N: 91 Object:(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source) Stat:is completely incorporated in Simbad Note:SCUBA at JCMT maps of the submm dust emission from the Perseus molecular cloud: 91 embedded starless and protostellar cores and filamentary structures are found. See also [HFR2007]. in source:NAME Perseus Molecular Cloud Ref:=2005A&A...440..151H byHATCHELL J. , RICHER J.S., FULLER G.A., QUALTROUGH C.J., LADD E.F., CHANDLER C.J. Astron. Astrophys., 440, 151-161 (2005) Star formation in Perseus. Clusters, filaments and the conditions for star formation. oParagraph 5.1 IRAS 03422+3256 is a probable misprint for IRAS 03422+3156. oTable A1: <[HRF2005] NN> (Nos 1-91). =E=Catalogue in electronic form as J/A+A/440/151 Originof the Acronym: S = Created by Simbad, the CDS Database
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