Tom Quinn
Affiliations: | University of Washington, Seattle, Seattle, WA |
Area:
Astronomy and AstrophysicsGoogle:
"Tom Quinn"Mean distance: 13975
Collaborators
Sign in to add collaborator| David L G Noakes | collaborator | University of Washington (Evolution Tree) |
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Publications
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| Ricarte A, Tremmel M, Natarajan P, et al. (2020) A Link between Ram Pressure Stripping and Active Galactic Nuclei The Astrophysical Journal. 895: L8 |
| Sanchez NN, Werk JK, Tremmel M, et al. (2019) Not So Heavy Metals: Black Hole Feedback Enriches the Circumgalactic Medium The Astrophysical Journal. 882: 8 |
| Byrne L, Christensen C, Tsekitsidis M, et al. (2019) Implementing Dust Shielding as a Criteria for Star Formation The Astrophysical Journal. 871: 213 |
| Christensen CR, Davé R, Brooks AM, et al. (2018) Tracing Outflowing Metals in Simulations of Dwarf and Spiral Galaxies The Astrophysical Journal. 867: 142 |
| Dunn G, Bellovary J, Holley-Bockelmann K, et al. (2018) Sowing Black Hole Seeds: Direct Collapse Black Hole Formation with Realistic Lyman–Werner Radiation in Cosmological Simulations The Astrophysical Journal. 861: 39 |
| Sanchez NN, Bellovary JM, Holley-Bockelmann K, et al. (2018) Preferential Accretion in the Supermassive Black Holes of Milky Way-size Galaxies Due to Direct Feeding by Satellites The Astrophysical Journal. 860: 20 |
| Clarke AJ, Debattista VP, Roškar R, et al. (2017) The origin of type I profiles in cluster lenticulars: an interplay between ram pressure stripping and tidally induced spiral migration Monthly Notices of the Royal Astronomical Society. 465 |
| Harris KA, Debattista VP, Governato F, et al. (2017) Quantifying the origin and distribution of intracluster Light in a Fornax-Like Cluster Monthly Notices of the Royal Astronomical Society. 467: 4501-4513 |
| Szulágyi J, Mayer L, Quinn T. (2017) Circumplanetary discs around young giant planets: a comparison between core-accretion and disc instability Monthly Notices of the Royal Astronomical Society. 464: 3158-3168 |
| Tomozeiu M, Mayer L, Quinn T. (2016) TIDAL STIRRING of SATELLITES with SHALLOW DENSITY PROFILES PREVENTS THEM from BEING TOO BIG to FAIL Astrophysical Journal Letters. 827 |