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WVU astrophysicists part of gravitational wave search that provides insights into galaxy evolution and mergers
WVU astrophysicists gravitational wave search galaxy evolution and mergers
2016/4/13
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 ...
A Bayesian Approach to Locating the Red Giant Branch Tip Magnitude (Part I)
Bayesian Approach Locating Giant Branch Tip Magnitu
2011/10/10
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: A large HI shell in the outer part of the Galaxy
ISM bubbles — ISM kinematics and dynamics —ISM structure —supernova remnants
2010/11/10
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.
The Multi-wavelength Extreme Starburst Sample of Luminous Galaxies Part I: Sample Characteristics
Galaxy Astrophysics (astro-ph.GA)
2010/12/28
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?
Fabry-perot kinematics orion nebula hh 202-204
2009/6/10
Fabry-perot kinematics of hh 202-204 in the orion nebula:are they part of a big bipolar outflow?
STARK BROADENING PARAMETER TABLES FOR In II (Part II)
II multiplets STARK BROADENING PARAMETER TABLES
2009/3/16
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...
THIRD DERIVATIVES OF THE INTEGRABLE PART OF AN ASTEROID HAMILTONIAN
Celestial mechanics-Minor planets asteroids
2009/2/16
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 ...
Durham University part of international team to win Descartes prize
cosmic rays Stereoscopic System
2007/3/28