GAL 048.99-00.29 , the SIMBAD biblio

GAL 048.99-00.29 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:43:57


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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.
1994A&A...291..261C viz 38 39 The occurrence of H2O masers in HII regions. CODELLA C., FELLI M., NATALE V., et al.
1994ApJ...436..117K 76 91 Kinematic distances of galactic HII regions from H I absorption studies. KUCHAR T.A. and BANIA T.M.
1997ApJ...488..224K viz 760 101 All-sky 4.85 GHz flux measurements of H II regions. KUCHAR T.A. and CLARK F.O.
2004MNRAS.355..899C 95 41 MSX mid-infrared imaging of massive star birth environments - II. Giant HII regions. CONTI P.S. and CROWTHER P.A.
2006ApJS..165..338Q viz 15       D               149 58 Radio recombination lines in galactic H II regions. QUIREZA C., ROOD R.T., BALSER D.S., et al.
2006ApJ...653.1226Q viz 15       D               1 156 129 The electron temperature gradient in the galactic disk. QUIREZA C., ROOD R.T., BANIA T.M., et al.
2012ApJ...752..146L viz 15       D               2 775 42 Milky Way star-forming complexes and the turbulent motion of the Galaxy's molecular gas. LEE E.J., MURRAY N. and RAHMAN M.
2015PASJ...67...65N 2730 T   A D     X C       69 9 1 Astrometry of Galactic star-forming regions
G48.99-0.30 and G49.19-0.34 with VERA : Astrometric accuracy verification of VERA.
NAGAYAMA T., KOBAYASHI H., OMODAKA T., et al.
2017RAA....17...47H 22 ~ Ionized gas clouds near the Sagittarius Arm tangent. HOU L.-G., DONG J., GAO X.-Y., et al.
2018AJ....155..204R 41           X         1 46 48 Revised distances to 21 supernova remnants. RANASINGHE S. and LEAHY D.A.
2019ApJ...874...94W 180       D     X C       4 24 27 Trigonometric parallaxes of star-forming regions beyond the tangent point of the Sagittarius spiral arm. WU Y.W., REID M.J., SAKAI N., et al.
2023ApJS..268...56Z viz 17       D               2 247 ~ A Systematic Observational Study on Galactic Interstellar Ratio 18O/17O. II. C18O and C17O J = 2-1 Data Analysis. ZOU Y.P., ZHANG J.S., HENKEL C., et al.

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