papers

Publications (10)

astro-ph2004

LFVN observations of active galactic nuclei

A. Pushkarev, I. Molotov, M. Nechaeva +7

In November 1999 we carried out VLBI observations of several quasars and BL Lacertae objects at 1.66 GHz. Six antennas participated in the experiment (Bear Lakes, Svetloe, Pushchin…

astro-ph.SR2020

COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2

J. C. Morford, D. M. Fenech, R. K. Prinja +12

The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechani…

astro-ph.GA2023

The Co-Ordinated Radio and Infrared Survey for High-Mass Star Formation. V. The CORNISH-South Survey and Catalogue

T. Irabor, M. G. Hoare, M. Burton +32

We present the first high spatial resolution radio continuum survey of the southern Galactic plane. The CORNISH project has mapped the region defined by $295^{\circ} < l < 350^{\ci…

astro-ph.IM2023

Inspecting spectra with sound: proof-of-concept & extension to datacubes

James W. Trayford, C. M. Harrison, R. C. Hinz +3

We present a novel approach to inspecting galaxy spectra using sound, via their direct audio representation ('spectral audification'). We discuss the potential of this as a complem…

astro-ph2000

Measuring the Size of the Vela Pulsar's Radio Emission Region

C. R. Gwinn, J. E. Reynolds, D. L. Jauncey +9

We describe measurements of the size of the Vela pulsar via scintillation, using both fits to the distribution of intensity and measurements of the modulation index. We briefly dis…

astro-ph.SR2016

ALMA observations of the supergiant B[e] star Wd1-9

D. Fenech, J. S. Clark, R. K. Prinja +3

Mass-loss in massive stars plays a critical role in their evolution, although the precise mechanism(s) responsible - radiatively driven winds, impulsive ejection and/or binary inte…

astro-ph.SR2012

Size of the Vela Pulsar's Emission Region at 18 cm Wavelength

C. R. Gwinn, M. D. Johnson, J. E. Reynolds +12

We present measurements of the linear diameter of the emission region of the Vela pulsar at observing wavelength lambda=18 cm. We infer the diameter as a function of pulse phase fr…

astro-ph.IM2012

Noise in the Cross-Power Spectrum of the Vela Pulsar

C. R. Gwinn, M. D. Johnson, J. E. Reynolds +12

We compare the noise in interferometric measurements of the Vela pulsar from ground- and space-based antennas with theoretical predictions. The noise depends on both the flux densi…

astro-ph.CO2012

A tidal disruption-like X-ray flare from the quiescent galaxy SDSS J120136.02+300305.5

R. D. Saxton, A. M. Read, P. Esquej +4

SDSS J120136.02+300305.5 was detected in an XMM-Newton slew from June 2010 with a flux 56 times higher than an upper limit from ROSAT, corresponding to Lx~3x10^44 ergs/s. It has th…

astro-ph.SR2018

An ALMA 3mm continuum census of Westerlund 1

D. M. Fenech, J. S. Clark, R. K. Prinja +6

Massive stars play an important role in both cluster and galactic evolution and the rate at which they lose mass is a key driver of both their own evolution and their interaction w…