This article has an erratum: [https://doi.org/10.1051/0004-6361/201015938e]
Volume 526, February 2011
|Number of page(s)||12|
|Published online||10 January 2011|
The Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) survey
I. Survey description and pilot observations
Netherlands Institute for Radio Astronomy (ASTRON),
2 University of New Mexico, 800 Yale Blvd, Albuquerque, NM, USA
3 Astronomy Department, Bologna University, via Ranzani 1, 40127 Bologna, Italy
4 Kapteyn Astronomical Institute, Postbus 800, 9700 AV Groningen, The Netherlands
5 Department of Astronomy, New Mexico State University, PO Box 30001, MSC 4500, Las Cruces, NM 88003, USA
6 Astronomisches Institut der Ruhr-Universität Bochum, Universitätsstr. 150, 44780 Bochum, Germany
7 Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, 9000 Ghent, Belgium
Received: 15 October 2010
Accepted: 27 November 2010
We introduce a new, very deep neutral hydrogen (H i) survey being performed with the Westerbork Synthesis Radio Telescope (WSRT). The Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) Survey is producing an archive of some of the most sensitive H i observations available, on the angular scales which are most useful for studying faint, diffuse gas in and around nearby galaxies. The survey data are being used to perform careful modeling of the galaxies, characterizing their gas content, morphology, and kinematics, with the primary goal of revealing the global characteristics of cold gas accretion onto spiral galaxies in the local Universe. In this paper, we describe the survey sample selection, the data acquisition, reduction, and analysis, and present the data products obtained during our pilot program, which consists of UGC 2082, NGC 672, NGC 925, and NGC 4565. The observations reveal a first glimpse of the picture that the full HALOGAS project aims to illuminate: the properties of accreting H i in different types of spirals, and across a range of galactic environments. None of the pilot survey galaxies hosts an H i halo of the scale of NGC 891, but all show varying indications of halo gas features. We compare the properties of detected features in the pilot survey galaxies with their global characteristics, and discuss similarities and differences with NGC 891 and NGC 2403.
Key words: galaxies: spiral / galaxies: evolution / galaxies: ISM / galaxies: halos / galaxies: kinematics and dynamics
© ESO, 2011
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.