2011MNRAS.411.2059C


Query : 2011MNRAS.411.2059C

2011MNRAS.411.2059C - Mon. Not. R. Astron. Soc., 411, 2059-2066 (2011/March-1)

Blueshifted outflow from 24.329+0.145.

CASWELL J.L. and GREEN J.A.

Abstract (from CDS):

New studies of an hydroxyl (OH) maser site that has puzzled astronomers for more than 40 yr demonstrate that its emission arises in a unique strong blueshifted outflow. Measurements with the Australia Telescope Compact Array (ATCA) locate this enigmatic OH 1667-MHz maser at 24.329+0.145 (Galactic coordinates). This is coincident (to arcsecond accuracy) with maser emission at the 6668-MHz transition of methanol and a newly discovered maser at the 22-GHz transition of water. The methanol maser establishes the site as one of high-mass star formation, and the small spread of methanol features about a median velocity of +113 km/s defines its systemic velocity. The water maser shows a combination of some emission arising near this systemic velocity, and the remainder arising in the blueshifted outflow.

The 1667-MHz OH emission extends over more than 20 km/s, and our demonstrated association with the methanol maser reveals that this is offset from the systemic velocity by as much as 50 km/s. The implied energetic blueshifted outflow is unprecedented in OH masers of this class. Our spectral studies using the ATCA, with a new high-resolution spectrometer, achieve full polarization observations of the 1665- and 1667-MHz OH ground-state transitions. The dominance of 1667-MHz emission, with no detection at 1665 MHz, suggests unusual physical properties in the ouflow region. Likewise, the prevalence of linear polarization may be a consequence of emission arising in a fast-moving outflow, with perhaps a link between linear polarization orientation and outflow orientation.

We also present new observations of maser sites 24.494-0.039 and 24.790+0.083. These close neighbours of 24.329+0.145, with methanol maser emission at a similar systemic velocity, are also accompanied by masers of water and OH, but have no unusual maser properties. The velocity and Galactic longitude of all three sites, and of the H II complex W42, correspond to an especially interesting Galactic location near the tangent point of the 3-kpc arm (expanding ring), at a distance of 7.7 kpc.


Abstract Copyright: 2010 The Author Monthly Notices of the Royal Astronomical Society2010 RAS

Journal keyword(s): masers - stars: formation - H {sc ii} regions - ISM: molecules - Galaxy: kinematics and dynamics - radio lines: ISM

Simbad objects: 4

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Number of rows : 4
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 [M91] B183232.3-073824 Mas 18 35 09.4 -07 34 58           ~ 11 0
2 [VGM95] 183323.3-073350 Mas 18 36 05.8 -07 31 19           ~ 5 0
3 Caswell OH 024.78+00.08 Mas 18 36 12.5 -07 12 10           ~ 18 0
4 GRS G024.80 +00.10 SFR 18 38 14.8 -06 47 39           ~ 120 0

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