2000ApJ...544L.153G


Query : 2000ApJ...544L.153G

2000ApJ...544L.153G - Astrophys. J., 544, L153-L156 (2000/December-1)

A subarcsecond binary radio source associated with the X-ray-emitting young stellar object YLW 15.

GIRART J.M., RODRIGUEZ L.F. and CURIEL S.

Abstract (from CDS):

YLW 15 is a remarkable object since it exhibits phenomena, such as strong millimeter emission and association with a bipolar outflow, that characterize extremely young stars (class 0 or I objects) while at the same time presenting strong, time-variable X-ray emission that is ubiquitous and detected characteristically in more evolved objects. Our Very Large Array observations reveal that YLW 15 is a subarcsecond (0".6) radio binary, with one of the components spatially extended and the other unresolved. We discuss the possibility that the components of the binary system may have different characteristics also at other wavelengths, possibly as a result of different evolutionary status, and discuss future observations that may test this hypothesis.

Abstract Copyright: ∼

Journal keyword(s): ISM: Individual: Alphanumeric: YLW 15 - ISM: Jets and Outflows - Stars: Formation - X-Rays: ISM

Nomenclature: Table 1, Fig.1: [GRC2000] VLA N (Nos 1-2).

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IRAS 05435-0011 Y*O 05 46 08.45544 -00 10 02.9568           ~ 91 0
2 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
3 YLW 15 Y*O 16 27 26.906 -24 40 50.81           ~ 281 1
4 [GCR2002] L1681B VLA 2 Rad 16 27 26.911 -24 40 51.40           ~ 19 0
5 YLW 16 IR 16 27 28 -24 39.5           ~ 19 0
6 LDN 1681B DNe 16 27 35.7 -24 43 26           ~ 27 0
7 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
8 NVSS J162914-300003 Rad 16 29 14.887 -30 00 01.93           ~ 7 1

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