His primary areas of investigation include Astrophysics, Galaxy, Galaxy rotation curve, Astronomy and Dark matter. His Astrophysics study is mostly concerned with Surface brightness, Elliptical galaxy, Surface brightness fluctuation, Luminous infrared galaxy and Low-surface-brightness galaxy. Stacy S. McGaugh has included themes like Fundamental plane and Dark galaxy in his Surface brightness fluctuation study.
Many of his studies on Galaxy involve topics that are commonly interrelated, such as Baryon. The study incorporates disciplines such as Dark fluid, Cold dark matter, Dark matter halo and Structure formation in addition to Galaxy rotation curve. His study in Dark matter is interdisciplinary in nature, drawing from both Radius, Newtonian dynamics, Modified Newtonian dynamics, Spiral galaxy and Gravitation.
Stacy S. McGaugh mainly investigates Astrophysics, Galaxy, Astronomy, Dark matter and Surface brightness. Galaxy rotation curve, Halo, Baryon, Elliptical galaxy and Star formation are the subjects of his Astrophysics studies. His work in Galaxy rotation curve addresses subjects such as Dark matter halo, which are connected to disciplines such as Scalar field dark matter and Hot dark matter.
He combines topics linked to Stars with his work on Galaxy. He combines subjects such as Cosmology, Modified Newtonian dynamics, Newtonian dynamics and Gravitation with his study of Dark matter. His Surface brightness research integrates issues from Brightness, Low-surface-brightness galaxy, Metallicity and Photometry.
Stacy S. McGaugh focuses on Astrophysics, Galaxy, Dark matter, Galaxy rotation curve and Astronomy. His Astrophysics and Stellar mass, Milky Way, Baryon, Halo and Galaxy formation and evolution investigations all form part of his Astrophysics research activities. In Galaxy, Stacy S. McGaugh works on issues like Stars, which are connected to Tidal force and Line.
His Dark matter research is multidisciplinary, incorporating perspectives in Gravitation, Modified Newtonian dynamics, Angular momentum and Velocity dispersion. His Galaxy rotation curve study combines topics from a wide range of disciplines, such as Dark matter halo, Stellar population, Photometry, Spiral galaxy and Gravitational field. His Tully–Fisher relation research incorporates themes from Population synthesis and Disc galaxy.
His primary scientific interests are in Astrophysics, Galaxy, Dark matter, Galaxy rotation curve and Stellar mass. His Baryon, Tully–Fisher relation, Milky Way, Dwarf galaxy and Surface brightness study are his primary interests in Astrophysics. His work in Surface brightness addresses issues such as Stars, which are connected to fields such as Star and Brightness.
He frequently studies issues relating to Acceleration and Galaxy. His Dark matter research is within the category of Astronomy. His work carried out in the field of Galaxy rotation curve brings together such families of science as Photometry, Dark matter halo and Spiral galaxy.
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Modified Newtonian dynamics as an alternative to dark matter
Robert H. Sanders;Stacy S. McGaugh.
Annual Review of Astronomy and Astrophysics (2002)
The Baryonic Tully-Fisher Relation
Stacy McGaugh;Jim Schombert;Greg Bothun;Erwin de Blok.
arXiv: Astrophysics (2000)
Modified Newtonian Dynamics (MOND):Observational Phenomenology and Relativistic Extensions
Benoît Famaey;Benoît Famaey;Stacy S. McGaugh;Stacy S. McGaugh.
Living Reviews in Relativity (2012)
H II region abundances - Model oxygen line ratios
Stacy S. McGaugh.
The Astrophysical Journal (1991)
The Baryonic Tully-Fisher Relation.
S. S. McGaugh;J. M. Schombert;G. D. Bothun;W. J. G. de Blok.
The Astrophysical Journal (2000)
Mass Density Profiles of LSB Galaxies
W.J.G. de Blok;Stacy S. McGaugh;Albert Bosma;Vera C. Rubin.
arXiv: Astrophysics (2001)
Mass Density Profiles of Low Surface Brightness Galaxies
W. J. G. de Blok;Stacy S. McGaugh;Albert Bosma;Vera C. Rubin.
The Astrophysical Journal (2001)
THE BARYONIC TULLY-FISHER RELATION OF GALAXIES WITH EXTENDED ROTATION CURVES AND THE STELLAR MASS OF ROTATING GALAXIES
Stacy S. McGaugh.
The Astrophysical Journal (2005)
The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND
arXiv: Cosmology and Nongalactic Astrophysics (2011)
The dark and visible matter content of low surface brightness disc galaxies
W. J. G. de Blok;Stacy S. McGaugh.
Monthly Notices of the Royal Astronomical Society (1997)
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