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| IRAS 13039-6108 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:28:16 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
1988IRASP.C......0J 
|
14 | D | 1 | 245223 | ~ | Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 | JOINT IRAS SCIENCE WORKING GROUP | ||
| 1990AJ.....99..303P | 56 | 26 | A search for young stellar objects in southern dark clouds. | PERSI P., FERRARI-TONIOLO M., BUSSO M., et al. | |||||
| 1990MmSAI..61...67P | 55 | ~ | A search for young stellar objects in southern dark clouds. | PERSI P., FERRARI-TONIOLO M., BUSSO M., et al. | |||||
|
2005A&A...432..921F
|
134 | 69 | Search for massive protostellar candidates in the southern hemisphere. I. Association with dense gas. | FONTANI F., BELTRAN M.T., BRAND J., et al. | |||||
| 2008ApJ...675L..33B | 23 | 40 | Ethynyl (C2H) in massive star formation: tracing the initial conditions? | BEUTHER H., SEMENOV D., HENNING T., et al. | |||||
| 2010A&A...520A.102M | 731 | D | X C | 19 | 54 | 21 | LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32. | MIETTINEN O. and HARJU J. | |
|
2011A&A...533A..17B
|
39 | X | 1 | 7 | 17 | The Coalsack near and far. | BEUTHER H., KAINULAINEN J., HENNING T., et al. | ||
| 2012A&A...540A.104M | 206 | D | X | 6 | 27 | 21 | A molecular line study of the filamentary infrared dark cloud G304.74+01.32. | MIETTINEN O. | |
|
2018A&A...609A.123M
|
185 | A | S X | 4 | 36 | 2 | The Seahorse Nebula: New views of the filamentary infrared dark cloud G304.74+01.32 from SABOCA, Herschel, and WISE. | MIETTINEN O. | |
| 2020A&A...639A..65M | 552 | D | X C | 13 | 22 | ~ | What did the seahorse swallow? APEX 170 GHz observations of the chemical conditions in the Seahorse infrared dark cloud. | MIETTINEN O. | |
| 2020A&A...644A..82M | 123 | X C | 2 | 29 | ~ | Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions. | MIETTINEN O. |
