Stacy McGaugh
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About
Stacy McGaugh is a Professor at Case Western Reserve University, located in the United States. His research areas focus on galaxy dynamics, particularly the Baryonic Tully–Fisher Relation and the accelerated structure formation of massive galaxies. Recent contributions include investigations into gas-rich low surface brightness galaxies and the application of new distance uncertainty schemes in galaxy flow models.
Recent Grants
Grant: Close
Vast Immensity, Exquisitely Made: Tidal Dwarf Galaxies and the Cosmic Dark Matter Problem
Open Date: 2014-09-01
Close Date: 2017-08-01
Grant: Close
The Relation between Mass and Light in Spiral Galaxies
Open Date: 2013-04-05
Close Date: 2015-04-04
Grant: Close
A FUNDAMENTAL PROPERTY OF GALAXIES IS THEIR MASS. HOW MUCH DO THEY WEIGH? HOW IS THEIR MASS DISTRIBUTED AMONGST DARK MATTER, STARS, AND OTHER BARYONIC MATTER? CAN WE MEASURE THE MASS FUNCTION? CAN THE BARYON FRACTIONS OF INDIVIDUAL OBJECTS BE RECONCILED W
Open Date: 2013-04-05
Close Date: 2015-04-04
Grant: Close
The Relation between Mass and Light in Spiral Galaxies
Open Date: 2011-04-01
Close Date: 2014-03-31
Grant: Close
The rotation curves of spiral galaxies provide some of the most compelling evidence for dark matter. These data also imply a close relationship between the luminous and dark components. One example is the Tully-Fisher (TF) relation between the luminosity
Open Date: 2011-04-01
Close Date: 2014-03-31
Articles (20)
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Collaborators (5)
Chris Mihos
Worcester R. and Cornelia B. Warner Professor of Astronomy
Case Western Reserve University
Tom Oosterloo
University of Groningen
James Schombert
Prof
Oregon State University
Albert Zijlstra
The University of Manchester
Filippo Fraternali
University of Groningen
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