activity
19972017
most citedDeceleration in the Expansion of SN1993J

79 citations · 247 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2017★ 43 cited

The population of SNe/SNRs in the starburst galaxy Arp 220. A self-consistent analysis of 20 years of VLBI monitoring

E. Varenius, J. E. Conway, F. Batejat +6

The nearby ultra-luminous infrared galaxy (ULIRG) Arp 220 is an excellent laboratory for studies of extreme astrophysical environments. For 20 years, Very Long Baseline Interferome…

astro-ph.CO2012★ 10 cited

Rapid variability of the compact radio sources in Arp220. Evidence for a population of microblazars?

F. Batejat, J. E. Conway, A. Rushton +3

Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previously identified as radio supernovae or supernova remnants. Aims. In order to sea…

astro-ph2004★ 45 cited

SiO masers in TX Cam: Simultaneous VLBA observations of two 43 GHz masers at four epochs

Jiyune Yi, R. S. Booth, J. E. Conway +1

We present the results of simultaneous high resolution observations of v=1 and v=2, J=1-0 SiO masers toward TX Cam at four epochs covering a stellar cycle. Near maser maximum (Epoc…

astro-ph2002

The Relative Spatial Distribution of SiO Masers in AGB Stars at 43 and 86 GHz

J. -F. Desmurs, R. Soria-Ruiz, F. Colomer +6

We present the first VLBI images of SiO masers in the circumstellar envelope of an S-type star obtained with the newly developed capabilities of the Very Long Baseline Array (VLBA)…

astro-ph1998★ 70 cited

VLBA Continuum Observations of NGC 4258: Constraints on an Advection-Dominated Accretion Flow

J. R. Herrnstein, L. J. Greenhill, J. M. Moran +4

We report a 3 sigma upper limit of 220 microJanskys on any 22-GHz continuum emission coincident with the central engine in NGC 4258. If NGC 4258 is powered by an advection-dominate…

astro-ph1997★ 79 cited

Deceleration in the Expansion of SN1993J

J. M. Marcaide, A. Alberdi, E. Ros +13

A rarity among supernova, SN 1993J in M81 can be studied with high spatial resolution. Its radio power and distance permit VLBI observations to monitor the expansion of its angular…