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[GRM93] G09.61+0.20 G , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST01:34:39 |
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 |
---|---|---|---|---|---|---|---|---|---|
2000A&A...359L...5T | 14 | 27 | Detection of the thermal radio continuum emission from the G9.62+0.19-F hot core. | TESTI L., HOFNER P., KURTZ S., et al. | |||||
2000A&A...362.1093M | 1 | 57 | 188 | VLBI observations of 6.7 and 12.2GHz methanol masers toward high mass star-forming regions. I. Observational results: protostellar disks or outflows? | MINIER V., BOOTH R.S. and CONWAY J.E. | ||||
2001ApJ...549..425H | 20 | 30 | A high-velocity molecular outflow from the G9.62+0.19 star-forming region. | HOFNER P., WIESEMEYER H. and HENNING T. | |||||
2003A&A...397..227P | 49 | 12 | Near and mid-infrared images of the massive star forming complex G9.62+0.19. | PERSI P., TAPIA M., ROTH M., et al. | |||||
2004ApJ...616..301G | 20 | 28 | High-velocity gas toward hot molecular cores: evidence for collimated outflows from embedded sources. | GIBB A.G., WYROWSKI F. and MUNDY L.G. | |||||
2005A&A...429..903L | 30 | 20 | The G9.62+0.19-F hot molecular core. The infrared view on very young massive stars. | LINZ H., STECKLUM B., HENNING T., et al. | |||||
2011ApJ...730..102L | 115 | X | 3 | 21 | 14 | Infall and outflow motions in the high-mass star-forming complex G9.62+0.19. | LIU T., WU Y., LIU S.-Y., et al. | ||
2017ApJ...849...25L | 41 | X | 1 | 30 | 19 | ALMA reveals sequential high-mass star formation in the G9.62+0.19 complex. | LIU T., LACY J., LI P.S., et al. | ||
2019A&A...626A..36D | 84 | F | 1 | 28 | ~ | ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19. | DALL'OLIO D., VLEMMINGS W.H.T., PERSSON M.V., et al. | ||
2020MNRAS.496.2790L | 230 | D | X | 6 | 165 | 41 | ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions - I. Survey description and a first look at G9.62+0.19. | LIU T., EVANS N.J., KIM K.-T., et al. |