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Query : 2019MNRAS.483.2014H |
2019MNRAS.483.2014H - Mon. Not. R. Astron. Soc., 483, 2014-2030 (2019/February-3)
Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293-2422.
HERNANDEZ-GOMEZ A., SAHNOUN E., CAUX E., WIESENFELD L., LOINARD L., BOTTINELLI S., HAMMAMI K. and MENTEN K.M.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): astrochemistry - ISM: molecules - stars: individual: (IRAS 16293-2422)
Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.
Simbad objects: 6
Number of rows : 6 |
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 Ophiuchus Molecular Cloud | SFR | 16 28 06 | -24 32.5 | ~ | 3628 | 1 | |||||
2 | IRAS 16293-2422 | cor | 16 32 22.56 | -24 28 31.8 | ~ | 1252 | 1 | |||||
3 | NAME IRAS 16293-2422B | Y*O | 16 32 22.63 | -24 28 31.8 | ~ | 283 | 0 | |||||
4 | NAME IRAS 16293-2422A | Y*O | 16 32 22.869 | -24 28 36.11 | ~ | 167 | 0 | |||||
5 | [QSR2011] Sgr B2(N)-SMA2 | cor | 17 47 19.885 | -28 22 13.29 | ~ | 93 | 0 | |||||
6 | NAME Sgr B2 | MoC | 17 47 20.4 | -28 23 07 | ~ | 2264 | 1 |
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