Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Quick Search
My eDoc
Session History
Support Wiki
Direct access to
document ID:

          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 606281.0, MPI für Astronomie / Publikationen_mpia
UWISH2 - the UKIRT widefield infrared survey for H2
Authors:Froebrich, D.; Davis, C. J.; Ioannidis, G.; Gledhill, T. M.; Takami, M.; Chrysostomou, A.; Drew, J.; Eislöffel, J.; Gosling, A.; Gredel, R.; Hatchell, J.; Hodapp, K. W.; Kumar, M. S. N.; Lucas, P. W.; Matthews, H.; Rawlings, M. G.; Smith, M. D.; Stecklum, B.; Varricatt, W. P.; Lee, H. T.; Teixeira, P. S.; Aspin, C.; Khanzadyan, T.; Karr, J.; Kim, H. J.; Koo, B. C.; Lee, J. J.; Lee, Y. H.; Magakian, T. Y.; Movsessian, T. A.; Nikogossian, E. H.; Pyo, T. S.; Stanke, T.
Date of Publication (YYYY-MM-DD):2011
Journal Abbrev.:Monthly Notices of the Royal Astronomical Society
Issue / Number:1
Start Page:480
End Page:492
Audience:Not Specified
Abstract / Description:We present the goals and preliminary results of an unbiased, near-infrared, narrow-band imaging survey of the first galactic quadrant (10° < l < 65°; -1?3 < b < +1?3). This area includes most of the giant molecular clouds and massive star forming regions in the Northern hemisphere. The survey is centred on the 1-0 S(1) rovibrational line of H2, a proven tracer of hot, dense molecular gas in star-forming regions, around evolved stars, and in supernova remnants. The observations complement existing and upcoming photometric surveys (Spitzer-GLIMPSE, UKIDSS-GPS, JCMT-JPS, AKARI, Herschel Hi-GAL, etc.), though we probe a dynamically active component of star formation not covered by these broad-band surveys. Our narrow-band survey is currently more than 60 per cent complete. The median seeing in our images is 0.73 arcsec. The images have a 5σ detection limit of point sources of KËœ 18 mag and the surface brightness limit is 10-19 W m-2 arcsec-2 when averaged over our typical seeing. Jets and outflows from both low- and high-mass young stellar objects are revealed, as are new planetary nebulae and - via a comparison with earlier K-band observations acquired as a part of the UKIDSS GPS - numerous variable stars. With their superior spatial resolution, the UWISH2 data also have the potential to reveal the true nature of many of the extended green objects found in the GLIMPSE survey.
Free Keywords:stars: formation; ISM: individual objects: Galactic Plane; ISM: jets and outflows; ISM: kinematics and dynamics; infrared: stars
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.