Issue |
A&A
Volume 471, Number 3, September I 2007
|
|
---|---|---|
Page(s) | L59 - L62 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20077782 | |
Published online | 16 July 2007 |
Letter to the Editor
Circumbinary molecular rings around young stars in Orion
1
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany e-mail: lzapata@mpifr-bonn.mpg.de
2
CRyA, Universidad Nacional Autónoma de México, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México
3
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
4
Academia Sinica Institute of Astronomy and Astrophysics, Taipei, Taiwan
Received:
1
May
2007
Accepted:
6
July
2007
We present high angular resolution 1.3 mm continuum, methyl
cyanide
molecular line, and 7 mm continuum observations made with the
Submillimeter Array and the Very Large Array, toward the most highly
obscured
and southern part of the massive star forming region OMC1S located behind
the
Orion Nebula. We find two flattened and rotating molecular structures with
sizes of a few hundred
astronomical units suggestive of circumbinary molecular rings produced by
the presence
of two stars with very compact circumstellar disks with sizes and separations of
about 50 AU, associated with the young stellar objects 139-409 and
134-411.
Furthermore, these two circumbinary rotating rings are related to two
compact and bright
hot molecular cores. The dynamic mass of the binary systems obtained from
our data
are ≥4 for 139-409 and ≥0.5
for 134-411.
This result supports the idea that intermediate-mass stars will form
through
circumstellar disks and jets/outflows, as the low mass stars do.
Furthermore, when intermediate-mass stars are in multiple systems
they seem to form a circumbinary ring similar to those seen
in young, multiple low-mass systems (e.g., GG Tau and UY Aur).
Key words: ISM: HII regions / ISM: jets and outflows / ISM: molecules / stars: formation / instrumentation: high angular resolution
© ESO, 2007
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