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| AGAL G328.961+00.566 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST12:30:40 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2014A&A...568A..41U 
|
16 | D | 1 | 10174 | 93 | ATLASGAL - Complete compact source catalogue: 280° <l< 60°. | URQUHART J.S., CSENGERI T., WYROWSKI F., et al. | ||
|
2014MNRAS.443.1555U
|
16 | D | 2 | 1184 | 176 | ATLASGAL - towards a complete sample of massive star forming clumps. | URQUHART J.S., MOORE T.J.T., CSENGERI T., et al. | ||
|
2015A&A...579A..91W
|
16 | D | 1 | 1616 | 97 | ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy. | WIENEN M., WYROWSKI F., MENTEN K.M., et al. | ||
|
2015ApJ...815..130G
|
16 | D | 1 | 3241 | 88 | Far-infrared dust temperatures and column densities of the MALT90 molecular clump sample. | GUZMAN A.E., SANHUEZA P., CONTRERAS Y., et al. | ||
|
2017AJ....154..140W
|
16 | D | 1 | 1806 | 9 | MALT90 kinematic distances to dense molecular clumps. | WHITAKER J.S., JACKSON J.M., RATHBORNE J.M., et al. | ||
|
2018MNRAS.473.1059U
|
16 | D | 1 | 8035 | 195 | ATLASGAL - properties of a complete sample of Galactic clumps. | URQUHART J.S., KONIG C., GIANNETTI A., et al. | ||
|
2016PASA...33...30R
|
16 | D | 1 | 3253 | 23 | Molecular Line Emission Towards High-Mass Clumps: The MALT90 Catalogue. | RATHBORNE J.M., WHITAKER J.S., JACKSON J.M., et al. | ||
|
2019MNRAS.487.1057D
|
17 | D | 1 | 376 | ~ | Beyond the solar circle - trends in massive star formation between the inner and outer galaxy. | DJORDJEVIC J.O., THOMPSON M.A., URQUHART J.S., et al. | ||
|
2022MNRAS.510.3389U
|
18 | D | 1 | 8770 | 20 | ATLASGAL - evolutionary trends in high-mass star formation. | URQUHART J.S., WELLS M.R.A., PILLAI T., et al. |
