... The Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands has been used to survey a section of the galactic plane at a radio frequency of 327MHz. ... Intensity data from the seperate epochs were combined, and the resulting images mosaiced to produce a single image of the entire survey region. ... The WSRT 327 MHz Galactic Plane Discrete Source Catalogue . ... It is available as a unix compressed Postscript file [164 Kbytes] and an ASCII text file [339 Kbytes]. ... Postscript [160 Kbytes] . ...

The H 2 O Southern Galactic Plane Survey (HOPS) has mapped a 100 degree strip of the Galactic plane (-70 > l > 30 , |b| < 0.5 ) using the 22-m Mopra antenna at 12-mm wavelengths. ... We have developed an automatic emission finding procedure based on the ATNF DUCHAMP software and have used it to create a new catalogue of 669 dense molecular clouds. ... Combined with other Galactic plane surveys this new molecular-line dataset constitutes a key tool for examining Galactic structure and evolution. ...

... X-Rays from the Galactic Plane . ... CXC , NASA Explanation: In February 2000, the orbiting Chandra X-ray Observatory spent 27 hours staring into the plane of our Milky Way galaxy . ... Intriguing is the diffuse blue glow of high energy x-rays, distinct from the individual sources in the picture. Astronomers have long debated whether our galactic plane's apparently extended x-ray emission was due to discrete sources or diffuse hot gas. ... Why does this energetic gas linger in the galactic plane? ...

. Cold clouds of hydrogen gas, from which stars may one day coalesce, reveal themselves to radio eyes as shadows against relatively warmer, brighter clouds behind them. We are studying these interstellar silhouettes with data from the Canadian Galactic Plane Survey and VLA Galactic Plane Survey . NAIC : . Steven Gibson , . Calgary : . Jeroen Stil , Russ Taylor . DRAO : . Peter Dewdney , Lloyd Higgs . Exeter : . Chris Brunt . UBC : . Bill McCutcheon . Hamburg : . Heinz Wendker . Maintained by Steven Gibson

... 2001 August 14 . X-Rays from the Galactic Plane . ... Explanation: In February 2000, the orbiting Chandra X-ray Observatory spent 27 hours staring into the plane of our Milky Way galaxy . ... Intriguing is the diffuse blue glow of high energy x-rays, distinct from the individual sources in the picture. Astronomers have long debated whether our galactic plane's apparently extended x-ray emission was due to discrete sources or diffuse hot gas. ... About APOD | ...

2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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... Now we're getting ready for the Australian SKA Pathfinder ( ASKAP ) and the Square Kilometre Array ( SKA ) itself. I co-lead the Galactic ASKAP survey, GASKAP, and the Polarisation survey, POSSUM. I have roles in SKA science planning, including membership on two SKA Science working groups (HI and The Galaxy), the SKA Science and Engineering Advisory Committee, Australia New Zealand SKA Coordination Committee (ANZSCC) and ANZSCC's Science Advisory Committee. ... Read More . ...

... An analysis on new observational data taken with the MPFS and SCORPIO spectrographs indicates that we are dealing with the "galactic wind": the gas is blown above the galactic plane with the characteristic velocity of about 130km/s. The gas outflow is caused by a combined action of winds from the supernovae and young massive stars located in the galaxy's circumnuclear region. ... The most probable hypothesis is that the accretion of intergalactic gas clouds is feeding their star formation. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...