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| [HRB81] W75N(Bc) , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST08:11:41 |
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More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 1994A&A...284..215H | 1 | 13 | 83 | Water masers embedded in ultracompact HII regions : the W 75N cloud core. | HUNTER T.R., TAYLOR G.B., FELLI M., et al. | ||||
| 1997ApJ...489..744T | 38 | 114 | A radio Jet-H2O maser system in W75N(B) at a 200 AU scale: exploring the evolutionary stages of young stellar objects. | TORRELLES J.M., GOMEZ J.F., RODRIGUEZ L.F., et al. | |||||
| 2003ApJ...584..882S | 56 | 45 | Clustered star formation in W75 N. | SHEPHERD D.S., TESTI L. and STARK D.P. | |||||
| 2004ApJ...601..952S | 28 | 29 | The nature of the massive young stars in W75 N. | SHEPHERD D.S., KURTZ S.E. and TESTI L. | |||||
2006A&A...445..971P 
|
22 | 15 | Mid-infrared images of the massive star forming region W75 N. | PERSI P., TAPIA M. and SMITH H.A. | |||||
| 2007MNRAS.380..246G | 52 | D | X | 2 | 34 | 26 | A high-frequency radio continuum study of massive young stellar objects. | GIBB A.G. and HOARE M.G. | |
| 2010AJ....139.2433C | 1017 | A | D | S X C F | 25 | 13 | 16 | A bright radio HH object with large proper motions in the massive star-forming region W75N. | CARRASCO-GONZALEZ C., RODRIGUEZ L.F., TORRELLES J.M., et al. |
| 2011A&A...527A..48S | 40 | X | 1 | 10 | 50 | The structure of the magnetic field in the massive star-forming region W75N. | SURCIS G., VLEMMINGS W.H.T., CURIEL S., et al. | ||
| 2020MNRAS.496.3128R | 1564 | A | D | S X C | 37 | 20 | 5 | Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B). | RODRIGUEZ-KAMENETZKY A., CARRASCO-GONZALEZ C., TORRELLES J.M., et al. |
| 2023ApJ...954...99Z | 174 | X | 4 | 20 | ~ | Submillimeter Observations of Magnetic Fields in Massive Star-forming Region W75N. | ZENG L., ZHANG Q., ALVES F.O., et al. |
