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HH 454 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.10.01CEST06:57:23 |
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 |
---|---|---|---|---|---|---|---|---|---|
1999AJ....118..972D | 28 | 30 | L1551 NE or L1551 IRS 5: which source drives HH 28/29 ? | DEVINE D., REIPURTH B. and BALLY J. | |||||
2000AJ....120.1449R | 49 | 140 | Hubble space telescope NICMOS images of Herbig-Haro energy sources: [Fe II] jets, binarity, and envelope cavities. | REIPURTH B., YU K.C., HEATHCOTE S., et al. | |||||
2000AJ....120.3177R | 83 | 185 | Disintegrating multiple systems in early stellar evolution. | REIPURTH B. | |||||
2002A&A...386..204F | 42 | K | 5 | 77 | Discovery of X-ray emission from the protostellar jet L1551 IRS5 (HH 154). | FAVATA F., FRIDLUND C.V.M., MICELA G., et al. | |||
2002AJ....124.1045R | 48 | 106 | Radio continuum maps of deeply embedded protostars: thermal jets, multiplicity, and variability. | REIPURTH B., RODRIGUEZ L.F., ANGLADA G., et al. | |||||
2003ApJ...595..266Y | 17 | 19 | High angular resolution, sensitive CS J = 2-1 and J = 3-2 imaging of the protostar L1551 NE: evidence for outflow-triggered star formation?. | YOKOGAWA S., KITAMURA Y., MOMOSE M., et al. | |||||
2004ApJS..154..346R | 16 | 16 | Models for the infrared cavity of HH 46/47. | RAGA A.C., NORIEGA-CRESPO A., GONZALEZ R.F., et al. | |||||
2006ApJ...645..357M | 47 | 38 | Multigenerational star formation in L1551. | MORIARTY-SCHIEVEN G.H., JOHNSTONE D., BALLY J., et al. | |||||
2006ApJ...649..280S | 28 | 26 | Entrainment mechanisms for outflows in the L1551 star-forming region. | STOJIMIROVIC I., NARAYANAN G., SNELL R.L., et al. | |||||
2011A&A...527A..41S ![]() |
39 | X | 1 | 184 | 15 | Dense gas and the nature of the outflows. | SEPULVEDA I., ANGLADA G., ESTALELLA R., et al. | ||
2011PASJ...63..921T | 39 | X | 1 | 21 | 10 | Skewed distributions and opposite velocity gradients of submillimeter molecular lines in low-mass protostellar envelopes. | TAKAKUWA S. and KAMAZAKI T. |
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