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GBS-VLA J053525.96-050543.3 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.29CET10:39:22 |
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 |
---|---|---|---|---|---|---|---|---|---|
2004AJ....127.1736R | 84 | 69 | Radio continuum jets from protostellar objects. | REIPURTH B., RODRIGUEZ L.F., ANGLADA G., et al. | |||||
2014ApJ...790...49K | 16 | D | 1 | 402 | 23 | The Gould's Belt Very Large Array survey. III. The Orion region. | KOUNKEL M., HARTMANN L., LOINARD L., et al. | ||
2017ApJ...840...36O | 382 | D | S X | 9 | 25 | 13 | Star formation under the outflow: the discovery of a non-thermal jet from OMC-2 FIR 3 and its relationship to the deeply embedded FIR 4 protostar. | OSORIO M., DIAZ-RODRIGUEZ A.K., ANGLADA G., et al. | |
2019ApJ...886....6T | 1396 | D | X C | 33 | 34 | 22 | The VLA/ALMA nascent disk and multiplicity (VANDAM) survey of Orion protostars. I. Identifying and characterizing the protostellar content of the OMC-2 FIR4 and OMC-2 FIR3 regions. | TOBIN J.J., MEGEATH S.T., VAN'T HOFF M., et al. | |
2021ApJS..255....2K | 44 | X | 1 | 70 | 3 | Mid-J CO line observations of protostellar outflows in the Orion molecular clouds. | KANG M., CHOI M., WYROWSKI F., et al. | ||
2022A&A...657A..78C | 45 | X | 1 | 60 | 13 | Organic chemistry in the protosolar analogue HOPS-108: Environment matters. | CHAHINE L., LOPEZ-SEPULCRE A., NERI R., et al. | ||
2022A&A...667A...6C | 1012 | A | S X C | 21 | 20 | 1 | OMC-2 FIR 4 under the microscope: Shocks, filaments, and a highly collimated jet at 100 au scales. | CHAHINE L., LOPEZ-SEPULCRE A., PODIO L., et al. | |
2023ApJ...944...92S | 205 | D | X | 5 | 27 | 2 | ALMA Fragmented Source Catalog in Orion (FraSCO). I. Outflow Interaction within an Embedded Cluster in OMC-2/FIR 3, FIR 4, and FIR 5. | SATO A., TAKAHASHI S., ISHII S., et al. | |
2023A&A...671A..35L | 280 | X C | 5 | 16 | ~ | SOLIS XVII. Jet candidate unveiled in OMC-2 and its possible link to the enhanced cosmic-ray ionisation rate. | LATTANZI V., ALVES F.O., PADOVANI M., et al. |