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MLLA 895 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.26CEST10:51:51 |
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 |
---|---|---|---|---|---|---|---|---|---|
1994ApJ...421..517P | 330 | 253 | HST photometry of the Trapezium cluster. | PROSSER C.F., STAUFFER J.R., HARTMANN L., et al. | |||||
1997AJ....113.1733H | 1616 | 923 | On the stellar population and star-forming history of the Orion Nebula Cluster. | HILLENBRAND L.A. | |||||
1998AJ....116.1816H | 1592 | 240 | Circumstellar disks in the Orion nebula cluster. | HILLENBRAND L.A., STROM S.E., CALVET N., et al. | |||||
2000ApJ...540..236H | 831 | 286 | Constraints on the stellar/substellar mass function in the inner Orion nebula cluster. | HILLENBRAND L.A. and CARPENTER J.M. | |||||
2002ApJ...573..366M | 1054 | 350 | The luminosity and mass function of the Trapezium cluster: from B stars to the deuterium-burning limit. | MUENCH A.A., LADA E.A., LADA C.J., et al. | |||||
2009A&A...502..883R | 15 | D | 1 | 2914 | 51 | Rotational studies in the Orion nebula cluster: from solar mass stars to brown dwarfs. | RODRIGUEZ-LEDESMA M.V., MUNDT R. and EISLOEFFEL J. | ||
2013AJ....146...85H | 16 | D | 1 | 1699 | 34 | An enhanced spectroscopic census of the Orion Nebula Cluster. | HILLENBRAND L.A., HOFFER A.S. and HERCZEG G.J. | ||
2014ApJ...782....8I | 16 | D | 2 | 148 | 6 | Near-infrared (JHK) spectroscopy of young stellar and substellar objects in Orion. | INGRAHAM P., ALBERT L., DOYON R., et al. | ||
2016ApJ...826...16E | 16 | D | 1 | 314 | 27 | Protoplanetary disks in the Orion OMC1 region imaged with ALMA. | EISNER J.A., BALLY J.M., GINSBURG A., et al. | ||
2016ApJ...831..155S | 16 | D | 1 | 927 | 3 | A VLA survey for faint compact radio sources in the Orion Nebula Cluster. | SHEEHAN P.D., EISNER J.A., MANN R.K., et al. | ||
2019A&A...626A..79P | 17 | D | 1 | 1887 | ~ | Do star clusters form in a completely mass-segregated way? | PAVLIK V., KROUPA P. and SUBR L. |