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On the heels of their participation in the historic research that resulted in the detection of gravitational waves, West Virginia University astrophysicists continue to plow new ground ...
We present a new approach for identifying the Tip of the Red Giant Branch (TRGB) which, as we show, works robustly even on sparsely populated targets. Moreover, the approach is highly adaptable to the...
GSH 91.5+ 2− 114 is a large HI shell located in the outer Galaxy at a kinematic distance of about 15 kpc. It was first identified in the Canadian Galactic Plane Survey (CGPS) by Pineault et al.
This paper introduces the Multi-wavelength Extreme Starburst Sample (MESS), a new catalog of 138 star-forming galaxies (0.1 < z < 0.3) optically selected from the SDSS using emission line strength dia...
Fabry-perot kinematics of hh 202-204 in the orion nebula:are they part of a big bipolar outflow?
Electron-, proton-, and ionized helium-impact broadening parameter tables for 101 In II multiplets, are presented as a function of temperature for the perturber density of 1016cm−3. Calculatio...
To apply the theorem of Nekhoroshev (1977) to asteroids, one ¯rst has to check whether a necessary geometrical condition is ful¯lled: either convexity, or quasi-convexity, or only a 3-jet ...
19 March 2007,An international team including physicists from Durham has won the coveted Descartes prize for Basic Research (worth £226,000) for its work studying some of the most violent phenom...

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