Journal
ASTROPHYSICAL JOURNAL
Volume 622, Issue 2, Pages L141-L144Publisher
IOP PUBLISHING LTD
DOI: 10.1086/429720
Keywords
infrared : stars; ISM : individual (W3 IRS 5); stars : formation
Categories
Ask authors/readers for more resources
We present Hubble Space Telescope NICMOS imaging of W3 IRS 5, a binary high-mass protostar. In addition to the two protostars, NICMOS images taken in the F222M and F160W filters show three new 2.22 mu m sources with very red colors; these sources fall within a region 5600 AU in diameter and are coincident with an similar to 100 M-circle dot, dense molecular clump. Two additional point sources are found within 0.'' 4 (800 AU) of one of the high-mass protostars; these may be stellar companions or unresolved emission knots from an outflow. We propose that these sources constitute a nascent Trapezium system in the center of the W3 IRS 5 cluster containing as many as five proto-OB stars. This would be the first identification of a Trapezium still deeply embedded in its natal gas.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available