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2014MNRAS.440..427R - Mon. Not. R. Astron. Soc., 440, 427-447 (2014/May-1)
A Herschel and BIMA study of the sequential star formation near the W 48A HII region.
RYGL K.L.J., GOEDHART S., POLYCHRONI D., WYROWSKI F., MOTTE F., ELIA D., NGUYEN-LUONG Q., DIDELON P., PESTALOZZI M., BENEDETTINI M., MOLINARI S., ANDRE Ph., FALLSCHEER C., GIBB A., DI GIORGIO A.M., HILL T., KONYVES V., MARSTON A., PEZZUTO S., RIVERA-INGRAHAM A., SCHISANO E., SCHNEIDER N., SPINOGLIO L., WARD-THOMPSON D. and WHITE G.J.
Abstract (from CDS):
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): stars: formation - ISM: clouds - dust, extinction - Hii regions - ISM: individual objects: W 48A - ISM: molecules
Nomenclature: Figs 2-3, Tables 2-3: [RGP2014] Clump H-N (Nos 1-3), [RGP2014] Core H-Na (Nos 2a-2b, 3a-3b).
CDS comments: The star forming region G35.80-1.38 in Figure A1 is not in Simbad.
Simbad objects: 26
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