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Query : 2021ApJ...910L...6T |
2021ApJ...910L...6T - Astrophys. J., 910, L6-L6 (2021/March-3)
The core mass function in the Orion Nebula Cluster region: what determines the final stellar masses?
TAKEMURA H., NAKAMURA F., KONG S., ARCE H.G., CARPENTER J.M., OSSENKOPF-OKADA V., KLESSEN R., SANHUEZA P., SHIMAJIRI Y., TSUKAGOSHI T., KAWABE R., ISHII S., DOBASHI K., SHIMOIKURA T., GOLDSMITH P.F., SANCHEZ-MONGE A., KAUFFMANN J., PILLAI T.G.S., PADOAN P., GINSBERG A., SMITH R.J., BALLY J., MAIRS S., PINEDA J.E., LIS D.C., BURKHART B., SCHILKE P., CHEN H.H.-H., ISELLA A., FRIESEN R.K., GOODMAN A.A. and HARPER D.A.
Abstract (from CDS):
Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.
Journal keyword(s): Star formation - Interstellar medium - Molecular clouds - Protostars - Radio observatories - CO line emission - Initial mass function
Simbad objects: 12
Number of rows : 12 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NAME Orion Nebula Cluster | OpC | 05 35.0 | -05 29 | ~ | 2334 | 0 | |||||
2 | NAME OMC-1 | MoC | 05 35 14 | -05 22.4 | ~ | 1170 | 2 | |||||
3 | OMC 3 | MoC | 05 35 20.0 | -05 01 00 | ~ | 273 | 1 | |||||
4 | OMC 2 | MoC | 05 35 27 | -05 10.1 | ~ | 450 | 1 | |||||
5 | OMC 4 | MoC | 05 36 06 | -05 35.7 | ~ | 71 | 0 | |||||
6 | NAME LDN 1641 North | HII | 05 36 17.6 | -06 22 10 | ~ | 239 | 0 | |||||
7 | BD-06 1253 | Ae* | 05 36 25.4320468080 | -06 42 57.684730284 | 11.65 | 10.9 | 10.29 | A1e | 435 | 1 | ||
8 | NAME Ori A | MoC | 05 38 | -07.1 | ~ | 3015 | 0 | |||||
9 | NAME Ori B | MoC | 05 41 43.0 | -01 54 44 | ~ | 1378 | 0 | |||||
10 | NAME Ophiuchus Molecular Cloud | SFR | 16 28 06 | -24 32.5 | ~ | 3634 | 1 | |||||
11 | NAME the Pipe Nebula | DNe | 17 30 | -25.0 | ~ | 403 | 1 | |||||
12 | SNR G012.8-00.2 | SFR | 18 14 14.0 | -17 55 50 | ~ | 258 | 0 |
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