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IRAS 23125+5921 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:36:05 |
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 |
---|---|---|---|---|---|---|---|---|---|
1986A&A...168..237W | 277 | 180 | H2O masers associated with IRAS sources in regions of star formation. | WOUTERLOOT J.G.A. and WALMSLEY C.M. | |||||
1988A&A...203..367W | 235 | 82 | Ammonia towards IRAS sources in the Orion and Cepheus clouds. | WOUTERLOOT J.G.A., WALMSLEY C.M. and HENKEL C. | |||||
1992AZh....69.1002K | 149 | 16 | A search for methanol masers at 44 GHz. | KALENSKIJ S.V., BACHILLER R., BERULIS I.I., et al. | |||||
1994AZh....71...37S | 150 | 7 | Detection of thermal methanol emission from 33 hot and cold clouds at 48 GHz. | SLYSH V.I., BACHILLER R., BERULIS I.I., et al. | |||||
1994PAZh...20..113K | 108 | ~ | The determination of methanol column density and abundance in molecular clouds from observations in the 1 0-0 0A+ line. | KALENSKII S.V. and SOBOLEV A.M. | |||||
1997A&AS..126..479G | 339 | 165 | Near infrared photometry of IRAS sources with colours like planetary nebulae. III. | GARCIA-LARIO P., MANCHADO A., PYCH W., et al. | |||||
2003A&A...399.1083K | 6715 | 27 | The association of IRAS sources and 12CO emission in the outer Galaxy. | KERTON C.R. and BRUNT C.M. | |||||
2004A&A...418..131K | 913 | 29 | Far-infrared loops in the 2nd Galactic Quadrant. | KISS C., MOOR A. and TOTH L.V. | |||||
2007PASJ...59.1185S | 15 | D | 1597 | 41 | Water maser and ammonia survey toward IRAS sources in the Galaxy. I. H2O maser data. | SUNADA K., NAKAZATO T., IKEDA N., et al. | |||
2011MNRAS.418.1689U | 15 | D | 1 | 596 | 139 | The red MSX source survey: ammonia and water maser analysis of massive star-forming regions. | URQUHART J.S., MORGAN L.K., FIGURA C.C., et al. | ||
2019ApJS..245...12O | 17 | D | 1 | 445 | ~ | The relationship between 6.7 GHz methanol masers and radio recombination lines in high-mass star-forming regions. | OUYANG X.-J., CHEN X., SHEN Z.-Q., et al. |