Laura Chomiuk
0000-0002-8400-3705
Michigan State University
49 papers found
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A New Model for the Radio Emission From Sn 1994i and an Associated Search for Radio Transients in M51
A MISSING-LINK IN THE SUPERNOVA–GRB CONNECTION: THE CASE OF SN 2012ap
The Distance to Nova V959 Mon From Vla Imaging
1fgl J1417.7–4407: A Likely Gamma-Ray Bright Binary With a Massive Neutron Star and a Giant Secondary
OPTICAL SPECTROSCOPIC OBSERVATIONS OFγ-RAY BLAZAR CANDIDATES. III. THE 2013/2014 CAMPAIGN IN THE SOUTHERN HEMISPHERE
RELATIVISTIC SUPERNOVAE HAVE SHORTER-LIVED CENTRAL ENGINES OR MORE EXTENDED PROGENITORS: THE CASE OF SN 2012ap
Radio Frequency Models of Novae in Eruption. I. The Free-Free Process in Bipolar Morphologies
1fgl J0523.5–2529: A New Probable Gamma-Ray Pulsar Binary
The 2011 OUTBURST OF RECURRENT NOVA T Pyx: X-Ray OBSERVATIONS EXPOSE THE WHITE DWARF MASS AND EJECTION DYNAMICS
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