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The Gould's Belt Very Large Array Survey V: The Perseus Region
Gerardo Pech, Laurent Loinard, Sergio A. Dzib +12
We present multi-epoch, large-scale ( 2000 arcmin), fairly deep ( 16 Jy), high-resolution ( 1") radio observations of the Perseus star-forming complex ob…
Shock-powered radio emission from V5589 Sagittarii (Nova Sgr 2012 1)
Jennifer H. S. Weston, J. L. Sokoloski, Laura Chomiuk +7
Since the Fermi discovery of -rays from novae, one of the biggest questions in the field has been how novae generate such high-energy emission. Shocks must be a fundamental ingr…
Non-Thermal Radio Emission from Colliding Flows in Classical Nova V1723 Aql
Jennifer H. S. Weston, J. L. Sokoloski, Brian D. Metzger +9
The importance of shocks in nova explosions has been highlighted by Fermi's discovery of γ-ray producing novae. Over three years of multi-band VLA radio observations of the 2010 no…
The Gould's Belt Very Large Array Survey II: The Serpens region
Gisela N. Ortiz-León, Laurent Loinard, Amy J. Mioduszewski +12
We present deep (Jy) radio continuum observations of the Serpens molecular cloud, the Serpens south cluster, and the W40 region obtained using the Very Large Array in it…
The Distance to Nova V959 Mon from VLA Imaging
J. D. Linford, V. A. R. M. Ribeiro, L. Chomiuk +7
Determining reliable distances to classical novae is a challenging but crucial step in deriving their ejected masses and explosion energetics. Here we combine radio expansion measu…