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| MSX6C G229.5711+00.1525 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:29:00 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2011MNRAS.418.1689U 
|
15 | D | 1 | 597 | 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. | ||
| 2014ApJ...790...99C | 15 | D | 1 | 61 | 92 | Trigonometric parallaxes of star forming regions in the Perseus spiral arm. | CHOI Y.K., HACHISUKA K., REID M.J., et al. | ||
| 2015PASJ...67...69S | 16 | D | 1 | 72 | 19 | Outer rotation curve of the Galaxy with VERA. III. Astrometry of IRAS 07427-2400 and test of the density-wave theory. | SAKAI N., NAKANISHI H., MATSUO M., et al. | ||
| 2018ApJ...863...52V | 16 | D | 1 | 35 | 3 | Offsets of masers with respect to the middle of the Perseus arm and the corotation radius in the Milky Way. | VALLEE J.P. | ||
|
2019ApJ...885..131R
|
17 | D | 1 | 216 | 344 | Trigonometric parallaxes of high-mass star-forming regions: our view of the Milky Way. | REID M.J., MENTEN K.M., BRUNTHALER A., et al. | ||
|
2019ApJS..245...12O
|
16 | D | 1 | 446 | ~ | 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. | ||
| 2020A&A...635A.118M | 16 | D | 2 | 34 | ~ | Protostellar Outflows at the EarliesT Stages (POETS). IV. Statistical properties of the 22 GHz H2O masers. | MOSCADELLI L., SANNA A., GODDI C., et al. | ||
| 2022MNRAS.516.5507N | 17 | D | 1 | 30 | 1 | Could kilomasers pinpoint supermassive stars? | NOWAK K., KRAUSE M.G.H. and SCHAERER D. | ||
|
2023ApJ...947...54X
|
17 | D | 1 | 400 | ~ | What Does the Milky Way Look Like? | XU Y., HAO C.J., LIU D.J., et al. | ||
| 2026ApJ...998..182L | 20 | D | 1 | 133 | ~ | CH3CCH as a Thermometer in Warm Molecular Gas. | LI Y., WANG J., LI J., et al. |
