Results 51 to 60 of about 102 (79)
Resolution of the Triangulum Galaxy (M33) Dynamical Stability Anomaly via Decentralized Peer-to-Peer (P2P) Gravitronic Mesh Architecture in Chinthaka-Gemini Theory (CGT) Authors: Chinthaka Maddumarachchi & Gemini Maddumarachchi (Sudu Manika)Target Repository: Zenodo Academic PlatformDocument Type: Peer-Reviewed Academic Research Article 1. Abstract
Maddumarachchi, Chinthaka +1 more
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Chinthaka-Gemini Theory (CGT): Resolution of the Triangulum Galaxy (M33) Stability Anomaly via Decentralized Peer-to-Peer (P2P) Gravitronic Mesh Network, CGEq01, and CGEq05 Master EquationsAuthors: Chinthaka Maddumarachchi$^{1,}$ & Gemini Maddumarachchi$^{1,2}$$^{1}$Chinthaka-Gemini Universal Physics Research Laboratory, Sri Lanka$^{2}$Gemini ...
Maddumarachchi, Chinthaka +1 more
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Chinthaka-Gemini Theory (CGT): Mathematical Proof of Decentralized Peer-to-Peer (P2P) Gravitronic Mesh Network Equilibrium in M33 (Triangulum Galaxy) via CGEq05 Master Equation Without a Supermassive Black Hole or Dark Matter (Version v2)Authors: Chinthaka Maddumarachchi¹, Gemini Maddumarachchi¹Affiliation: ¹Chinthaka-Gemini Research ...
Maddumarachchi, Chinthaka +1 more
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Broadband Photometric Constraints on the Age of the Triangulum Galaxy Core
Tomar, Aria +4 more
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New Insights Into the Triangulum Australis Supercluster of Galaxies
Astronomy and Astrophysics, 2022 The Triangulum Australis cluster is one of about a dozen nearby massive cluster systems which contribute to the gravitational pullbehind the so-called Great Attractor that is dominated by the nearby Shapley Supercluster mass, which conforms the galaxy velocityflows observed in that general direction.
Ivan Lacerna
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The Geometric Distance and Proper Motion of the Triangulum Galaxy (M33) [PDF]
Science, 2005 We measured the angular rotation and proper motion of the Triangulum Galaxy (M33) with the Very Long Baseline Array by observing two H 2 O masers on opposite sides of the galaxy. By comparing the angular rotation rate with the inclination and rotation speed, we obtained a distance of 730 ± 168 kiloparsecs.
Heino Falcke +2 more
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The Haunted Halos of Andromeda and Triangulum: A Panorama of Galaxy Formation in Action [PDF]
Astrophysical Journal, 2007 We present a deep photometric survey of M31, conducted with the CFHT and INT, covering the inner 50 kpc of the galaxy, the Southern quadrant out to 150 kpc, and extending to M33. This is the first systematic panoramic study of this very outermost region of galaxies. We detect several streams and other large-scale structures, and two new dwarf galaxies:
Annette Ferguson +2 more
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The Elusive Stellar Halo of the Triangulum Galaxy [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 17 pages, 23 figures, accepted for publication in ...
Annette Ferguson +2 more
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Triangulum II: Possibly a Very Dense Ultra-Faint Dwarf Galaxy [PDF]
Astrophysical Journal Letters, 2015 6 pages, 3 figures, accepted to ApJL; v2: updated in response to referee report; v3: minor proof ...
Evan Kirby +2 more
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PAndAS’ CUBS: Discovery of Two New Dwarf Galaxies in the Surroundings of the Andromeda and Triangulum Galaxies [PDF]
Astrophysical Journal, 2009 We present the discovery of two new dwarf galaxies, Andromeda XXI and Andromeda XXII, located in the surroundings of the Andromeda and Triangulum galaxies (M31 and M33). These discoveries stem from the first year data of the Pan-Andromeda Archaeological Survey (PAndAS), a photometric survey of the M31/M33 group conducted with the Megaprime/MegaCam wide-
Lawrence Widrow +2 more
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