Laura B. Chomiuk, Ph.D.
Affiliations: | 2010 | University of Wisconsin, Madison, Madison, WI |
Area:
Astronomy and Astrophysics, Elementary Particles and High Energy PhysicsGoogle:
"Laura Chomiuk"Mean distance: 17.84
Parents
Sign in to add mentorEric M. Wilcots | grad student | 2010 | UW Madison | |
(Supernova remnants across the Hubble sequence.) |
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Publications
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Kool EC, Johansson J, Sollerman J, et al. (2023) A radio-detected type Ia supernova with helium-rich circumstellar material. Nature. 617: 477-482 |
Li K, Strader J, Miller-Jones JCA, et al. (2020) The Flare-dominated Accretion Mode of a Radio-bright Candidate Transitional Millisecond Pulsar The Astrophysical Journal. 895: 89 |
Pellegrino C, Howell DA, Sarbadhicary SK, et al. (2020) Constraining the Source of the High Velocity Ejecta in the Type Ia SN 2019ein The Astrophysical Journal. 897: 159 |
Swihart SJ, Strader J, Urquhart R, et al. (2020) A New Likely Redback Millisecond Pulsar Binary with a Massive Neutron Star: 4FGL J2333.1–5527 The Astrophysical Journal. 892: 21 |
Rodriguez J, Urquhart R, Plotkin RM, et al. (2020) GS 2000+25: The Least Luminous Black Hole X-Ray Binary The Astrophysical Journal. 889: 58 |
Zhao Y, Heinke CO, Tudor V, et al. (2020) The MAVERIC survey: a hidden pulsar and a black hole candidate in ATCA radio imaging of the globular cluster NGC 6397 Monthly Notices of the Royal Astronomical Society. 493: 6033-6049 |
Sokolovsky KV, Mukai K, Chomiuk L, et al. (2020) X-ray spectroscopy of the γ-ray brightest nova V906 Car (ASASSN-18fv) Monthly Notices of the Royal Astronomical Society. 497: 2569-2585 |
Heinke CO, Ivanov MG, Koch EW, et al. (2020) The X-ray emissivity of low-density stellar populations Monthly Notices of the Royal Astronomical Society. 492: 5684-5708 |
Corbet RHD, Chomiuk L, Coe MJ, et al. (2019) Discovery of the Galactic High-mass Gamma-Ray Binary 4FGL J1405.1−6119 The Astrophysical Journal. 884: 93 |
Holoien TW, Vallely PJ, Auchettl K, et al. (2019) Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS The Astrophysical Journal. 883: 111 |