[ABB2014] WISE G035.040-00.500 , the SIMBAD biblio

[ABB2014] WISE G035.040-00.500 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:20:37


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
1982A&A...108..227W 116 141 Results of radio survey for new compact HII Regions. WINK J.E., ALTENHOFF W.J. and MEZGER P.G.
1986A&A...154L...8C 64 100 1.3 mm continuum observations of compact H II regions detected by IRAS I. CHINI R., KREYSA E., MEZGER P.G., et al.
1987A&A...181..378C 67 116 Dust emission and star formation in compact HII regions. CHINI R., KRUGEL E. and WARGAU W.
1989ApJS...71..469L viz 449 331 A survey of radio HII regions in the northern sky. LOCKMAN F.J.
1997ApJ...488..224K viz 760 101 All-sky 4.85 GHz flux measurements of H II regions. KUCHAR T.A. and CLARK F.O.
2001ApJ...549..979K 56 143 Radio continuum and recombination line study of ultracompact H II regions with extended envelopes. KIM K.-T. and KOO B.-C.
2012ApJ...752..146L viz 15       D               2 776 42 Milky Way star-forming complexes and the turbulent motion of the Galaxy's molecular gas. LEE E.J., MURRAY N. and RAHMAN M.
2012MNRAS.424.2442S viz 15       D               1 5154 176 The Milky Way Project First Data Release: a bubblier Galactic disc. SIMPSON R.J., POVICH M.S., KENDREW S., et al.
2014MNRAS.438..426H viz 16       D               1 834 10 A statistical study of gaseous environment of Spitzer interstellar bubbles. HOU L.G. and GAO X.Y.
2014PASJ...66...18P 236           X         6 9 ~ Studying the molecular ambient towards the young stellar object EGO G35.04-0.47. PARON S., ORTEGA M., ASTORT A., et al.
2016ApJ...831...73V viz 17       D               1 69 87 Star formation relations in the Milky Way. VUTISALCHAVAKUL N., EVANS II N.J. and HEYER M.
2019MNRAS.488.1141J viz 17       D               1 2612 20 The Milky Way Project second data release: bubbles and bow shocks. JAYASINGHE T., DIXON D., POVICH M.S., et al.

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