Issue |
A&A
Volume 586, February 2016
|
|
---|---|---|
Article Number | A34 | |
Number of page(s) | 5 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201527233 | |
Published online | 22 January 2016 |
Molecular jet emission and a spectroscopic survey of S235AB
1
Graduate School of Science and Engineering, Kagoshima
University,
1-21-35 Kôrimoto, 890-0065,
Kagoshima,
Japan
e-mail:
RossBurns88@Googlemail.com
2
Mizusawa VLBI Observatory, National Astronomical Observatory of
Japan, Osawa 2-21-1, Mitaka,
181-8588
Tokyo,
Japan
3
Department of Astronomical Sciences, SOKENDAI (Graduate University
for Advanced Studies), Osawa
2-21-1, Mitaka, 181-8588
Tokyo,
Japan
4
Mizusawa VLBI Observatory, National Astronomical Observatory of
Japan, 2-12 Hoshi-ga-oka,
Mizusawa-ku, Oshu-shi, 023-0861
Iwate,
Japan
Received: 24 August 2015
Accepted: 12 December 2015
Context. The S235AB star forming region houses a massive young stellar object which has recently been reported to exhibit possible evidence of jet rotation – an illusive yet crucial component of disk aided star formation theories.
Aims. We confirm the presence of a molecular counterpart to the jet and we also study the molecular environment in S235AB.
Methods. We search for velocity wings in the line emission of thermal SiO (J = 2–1, v = 0), a tracer of shocked gas, which would indicate the presence of jet activity. Utilising other lines detected in our survey we use the relative intensities of intra species transitions, isotopes, and hyperfine transitions to derive opacities, temperatures, column densities, and abundances of various molecular species in S235AB.
Results. The SiO (J = 2–1, v = 0) emission exhibits velocity wings of up to 75 km s-1 above and below the velocity of the star, indicating the presence of a jet. The molecular environment describes an evolutionary stage resembling a hot molecular core.
Key words: stars: massive / ISM: jets and outflows
© ESO, 2016
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.