GAL 024.49-00.04 , the SIMBAD biblio

GAL 024.49-00.04 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:06:05


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Title First 3 Authors
1989ApJS...71..469L viz 449 331 A survey of radio HII regions in the northern sky. LOCKMAN F.J.
1990A&AS...84..179C 408 163 The Arcetri atlas of H2O maser sources. COMORETTO G., PALAGI F., CESARONI R., et al.
1997ApJ...488..224K viz 760 101 All-sky 4.85 GHz flux measurements of H II regions. KUCHAR T.A. and CLARK F.O.
2002ApJS..143..469M 1 63 286 The physical conditions for massive star formation: dust continuum maps and modeling. MUELLER K.E., SHIRLEY Y.L., EVANS II N.J., et al.
2003ApJS..149..375S 74 203 A CS J=5⟶4 mapping survey toward high-mass star-forming cores associated with water masers. SHIRLEY Y.L., EVANS II N.J., YOUNG K.E., et al.
2007ApJ...669L..37W 60 29 Signatures of inflow motion in cores of massive star formation: potential collapse candidates. WU Y., HENKEL C., XUE R., et al.
2009MNRAS.392..170S 90       D     X         3 32 18 A multitransition molecular line study of inward motions towards massive star-forming cores. SUN Y. and GAO Y.
2009ChA&A..33...32Z 29 1 Characteristics of Massive Star-forming Molecular Cores: The Spectral Observations of 12CO, 13CO and C18O and the Statistical Comparison. ZHANG L.-Y. and GAO Y.
2010ApJ...719.1104R viz 203       D S   X C       4 79 28 A new sample of very massive star forming complexes in the Spitzer GLIMPSE survey. RAHMAN M. and MURRAY N.
2011ApJS..195....1R 91       D         F     8 32 27 The physical properties of high-mass star-forming clumps: a systematic comparison of molecular tracers. REITER M., SHIRLEY Y.L., WU J., et al.
2011AJ....142...94S viz 15       D               1 49 7 Testing the global star formation relation: an HCO+ (3-2) mapping study of red MSX sources in the Bolocam Galactic Plane Survey. SCHENCK D.E., SHIRLEY Y.L., REITER M., et al.
2012ApJ...752..146L viz 15       D               1 775 42 Milky Way star-forming complexes and the turbulent motion of the Galaxy's molecular gas. LEE E.J., MURRAY N. and RAHMAN M.

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