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| GRS G012.80 -00.20 , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:37:52 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1983A&AS...51..195H | 17 | 16 | Excitation conditions in HII regions. | HERTER T., HELFER H.L. and PIPHER J.L. | |||||
| 1983ApJ...265..791G | 1 | 3 | 27 | Molecular gas in the W 33 region. | GOLDSMITH P.F. and MAO X.-J. | ||||
| 1983ApJ...267..638H | 11 | 38 | Formation of OB clusters : W 33 complex. | HASCHICK A.D. and HO P.T.P. | |||||
| 1983PASAu...5..221G | 6 | 3 | The distribution of 115 GHz CO towards W 33. | GARDNER F.F., WHITEOAK J.B. and OTRUPCEK R.E. | |||||
| 1984A&A...138..131A | 39 | 14 | On the statistics of galactic HI clouds. | ANANTHARAMAIAH K.R., RADHAKRISHNAN V. and SHAVER P.A. | |||||
| 1986PASAu...6..504P | 4 | 3 | A southern hemisphere ammonia survey. | PETERS W.L., FORSTER J.R., GARDNER F.F., et al. | |||||
| 1988AZh....65..167L | 61 | 1 | Diagnostics of the solar wind transonic region. | LOTOVA N.A., NAGELIS Y.V., RUDNITSKIJ G.M., et al. | |||||
| 1988BAAS...20..983K | 2 | 0 | NH3 observations of post-shock molecular gas in ionization-shock fronts around W 33. | KETO E.R. and HO P.T.P. | |||||
| 1989ApJ...347..349K | 6 | 19 | NH3 observations of compressed postshock molecular gas in ionization-shock fronts around W 33. | KETO E.R. and HO P.T.P. | |||||
| 1999ARep...43..157V | 8 | 3 | The hot class I methanol maser W33Met. | VAL'TTS I.E. | |||||
| 2006A&A...460..721M | 54 | 23 | SiO and CH3CCH abundances and dust emission in high-mass star-forming cores. | MIETTINEN O., HARJU J., HAIKALA L.K., et al. | |||||
2010ApJS..186..406D 
|
92 | D | C | 2 | 80 | 79 | 350 µm polarimetry from the Caltech Submillimeter Observatory. | DOTSON J.L., VAILLANCOURT J.E., KIRBY L., et al. | |
|
2011MNRAS.411..705M
|
399 | D | S X C | 9 | 105 | 43 | Spectrophotometric distances to Galactic H II regions. | MOISES A.P., DAMINELI A., FIGUEREDO E., et al. |
