We describe one of the former, a 3D survey of the Gaactic plane at 21 cm.Wall, JasperUniversity of British ColumbiaGriffin, ElizabethHerzberg Astronomy & Astrophysics Research CentreJarrell, RichardYork UniversitySpringer, Cham
9 RegisterLog in Sign up with one click: Facebook Twitter Google Share on Facebook AcronymDefinition CGPSCollege of Graduate and Professional Studies(various universities) CGPSCanadian Galactic Plane Survey CGPSColumbia Grammar and Preparatory School(New York, New York) ...
Using observations made with the VLA, we have determined RMs for sources in regions of the Galactic plane not covered by the Canadian Galactic Plane Survey (CGPS) and Southern Galactic Plane Survey (SGPS). We have combined these new RMs with those determined from the CGPS and SGPS and have...
The Canadian Galactic Plane Survey has opened new vistas on the Milky Way, including cold hydrogen clouds that bridge a critical gap between the classical diffuse interstellar medium and the gravitationally bound molecular clouds that can form stars. The CGPS and its fellow IGPS surveys revealed ...
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G85.9−0.6, discovered with the Canadian Galactic Plane Survey (CGPS). High-resolution XMM- Newton images revealing the morphology of the diffuse emission, as well as discrete point sources, are presented and correlated with radio and Chandra images. The new data also permit a spectroscopic...
cGPS in GeoNetMiller, CraigCervelli, AnnieSurvey Quarterly
The Canadian Galactic Plane Survey (CGPS) is the largest effort of its kind to study and understand the Galactic Magnetic Field (GMF) and Interstellar Medium (ISM) in our Galaxy (see e.g. Taylor et al. 2003). The CGPS has mapped the Galactic plane visible from DRAO on all spatial ...
A shell-like structure, detectable at radio con-tinuum, infrared and neutral hydrogen wavelengths, is found to be associated with this star.M. ArnalS. CichowolskiJ. C. TestoriS. PineaultC. CappaConference on the Dynamic Interstellar medium: a Celebration of the Canadian Galactic Plane Survey...
Two new velocities for each region are independently measured using 1-arcminute resolution 21~cm HI and 2.6~mm $^{12}$CO line maps (from the Canadian Galactic Plane Survey and FCRAO Outer Galaxy Surveys) that show where gaseous shells are observed around the periphery of the ionized gas. ...