UWISH2 - the UKIRT Widefield Infrared Survey for H2
- Author(s)
- D. Froebrich, C. J. Davis, G. Ioannidis, T. M. Gledhill, M. Takami, A. Chrysostomou, J. Drew, J. Eislöffel, A. Gosling, R. Gredel, J. Hatchell, K. W. Hodapp, M. S. N. Kumar, P. W. Lucas, H. Matthews, M. G. Rawlings, M. D. Smith, B. Stecklum, W. P. Varricatt, H. T. Lee, P. S. Teixeira, C. Aspin, T. Khanzadyan, J. Karr, H.-J. Kim, B.-C. Koo, J. J. Lee, Y.-H. Lee, Tigran Yu. Magakian, T. A. Movsessian, Elena H. Nikogossian, T. S. Pyo, T. Stanke
- Abstract
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) ro-vibrational 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 5σdetection limit of point sources of K˜ 18 mag and the surface brightness limit is 110−19 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, theUWISH2 data also have the potential to reveal the true nature of many of the extended green objects found in the GLIMPSE survey.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Korea Astronomy and Space Science Institute, Joint ALMA Observatory, Max-Planck-Institut für Astronomie, Max-Planck-Institut für Radioastronomie, Universidade do Porto, University of Exeter, University of Kent, Joint Astronomy Centre, University of Hertfordshire, Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), No. 1, Section 4, Roosevelt Road, Imperial College London, Thüringer Landessternwarte Tautenburg, University of Oxford, University of Hawaii at Hilo, National Research Council Canada (NRC-CNRC), European Southern Observatory (Germany), Seoul National University (SNU), Byurakan Astrophysical Observatory, Subaru Telescope
- Journal
- Monthly Notices of the Royal Astronomical Society
- Volume
- 413
- Pages
- 480-492
- ISSN
- 0035-8711
- DOI
- https://doi.org/10.1111/j.1365-2966.2010.18149.x
- Publication date
- 05-2011
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Keywords
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/uwish2--the-ukirt-widefield-infrared-survey-for-h2(3a4143b2-a8ae-483c-ae0f-60c4aa275b8c).html