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Jansky Very Large Array GLObal view of the STAR formation in the Milky Way (GLOSTAR) survey. We aim to identify SNR candidates using continuum images from the Karl G. Radio spectral index, polarization, and emission at mid-infrared (MIR) wavelengths can help distinguish between SNRs and H II regions.Īims. However, SNRs are routinely confused with H II regions, which can have similar radio morphologies. Deep interferometric radio continuum surveys of the Galactic plane help in rectifying this apparent deficiency by identifying low surface brightness SNRs and compact SNRs that have not been detected in previous surveys. However, the completeness of the catalog of Galactic SNRs is expected to be only ~30%, with on order 700 SNRs yet to be detected. The properties of the population of Galactic supernova remnants (SNRs) are essential to our understanding of the dynamics of the interstellar medium (ISM) in the Milky Way.
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#Ghostnote dokara full
Here we show selected results for the first part of the survey, covering the range of 28° < l < 36° and | b |< 1°, including the full low-resolution continuum image, examples of high-resolution images of selected sources, and the first results from the spectral line data.Ĭontext. We also combined the D configuration images with the Effelsberg 100-m data to provide zero spacing information, and we jointly imaged the D- and B-configuration data for optimal sensitivity of the intermediate spatial ranges. This yielded spatial resolutions of 18″ and 1.5″ for the two configurations, respectively. The observations were conducted in the most compact D configuration of the VLA and in the more extended B configuration. In our observations we covered the radio continuum in full polarization, as well as the 6.7 GHz methanol maser line, the 4.8 GHz formaldehyde line, and seven radio recombination lines. We outline the main goals of the survey and give a detailed description of the observations and the data reduction strategy. This provides for the first time a radio survey covering all angular scales down to 1.5 arcsecond, similar to complementary near-IR and mid-IR galactic plane surveys. Jansky Very Large Array in the frequency range 4−8 GHz and the Effelsberg 100-m telescope. In this paper we give an overview of the GLOSTAR survey, a new survey covering large parts (145 square degrees) of the northern Galactic plane using the Karl G. Surveys of the Milky Way at various wavelengths have changed our view of star formation in our Galaxy considerably in recent years.
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