The first resolved imaging of milliarcsecond-scale jets in Circinus X-1
Monthly Notices of the Royal Astronomical Society: Letters 419:1 (2012)
Abstract:
We present the first resolved imaging of the milliarcsecond-scale jets in the neutron star X-ray binary Circinus X-1, made using the Australian Long Baseline Array. The angular extent of the resolved jets is ∼20mas, corresponding to a physical scale of ∼150au at the assumed distance of 7.8kpc. The jet position angle is relatively consistent with previous arcsecond-scale imaging with the Australia Telescope Compact Array. The radio emission is symmetric about the peak, and is unresolved along the minor axis, constraining the opening angle to be <20°. We observe evidence for outward motion of the components between the two halves of the observation. Constraints on the proper motion of the radio-emitting components suggest that they are only mildly relativistic, although we cannot definitively rule out the presence of the unseen, ultrarelativistic (Γ > 15) flow previously inferred to exist in this system. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.The pan-starrs-1 and the recent SN science
Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society 19 (2012) 166-172
Abstract:
The search for transient phenomena in the Universe has entered a new era. In the next decade new all-sky surveys will provide a vast amount of astronomical survey data. These data will address issues in many of the astronomical fields. In the Supernova field, we will have for the first time the possibility to discover SNe without most of the observational bias present in the previous SN searches. Here we report the status of the transients study in one of the new on-going all-sky surveys: the Panoramic Survey Telescope & Rapid Response System-1 (PanStarrs-1).A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc
Astronomy & Astrophysics EDP Sciences 537 (2012) a132
The VLT-FLAMES survey of massive stars: NGC 346-013 as a test case for massive close binary evolution⋆
Astronomy & Astrophysics EDP Sciences 537 (2012) a29
Application of a Bayesian Method to Absorption Spectral-Line Finding in Simulated ASKAP Data
Publications of the Astronomical Society of Australia Cambridge University Press (CUP) 29:3 (2012) 221-228