output
19982026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations

Showing 2019Show all

9 papers · 1 filter

astro-ph.GA2019★ 32 cited

Radio Observations of Supernova Remnant G1.9+0.3

Kieran J. Luken, Miroslav D. Filipović, Nigel I. Maxted +18

We present 1 to 10GHz radio continuum flux density, spectral index, polarisation and Rotation Measure (RM) images of the youngest known Galactic Supernova Remnant (SNR) G1.9+0.3, u…

astro-ph.GA2019★ 29 cited

The ASKAP-EMU Early Science Project:Radio Continuum Survey of the Small Magellanic Cloud

T. D. Joseph, M. D. Filipović, E. J. Crawford +53

We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images ar…

astro-ph.GA2019★ 61 cited

Probing the existence of very massive first stars

S. Salvadori, P. Bonifacio, E. Caffau +4

We present a novel approach aimed at identifying the key chemical elements to search for the (missing) descendants of very massive first stars exploding as Pair Instability Superno…

astro-ph.SR2019★ 55 cited

A massive white-dwarf merger product before final collapse

V. V. Gvaramadze, G. Gräfener, N. Langer +4

Gravitational wave emission can lead to the coalescence of close pairs of compact objects orbiting each other. For the case of neutron stars such mergers may yield masses above the…

astro-ph.SR2019★ 10 cited

On the long cycle variability of the Algol OGLE-LMC-DPV-065 and its stellar, orbital and disk parameters

R. E. Mennickent, M. Cabezas, G. Djurašević +13

OGLE-LMC-DPV-065 is an interacting binary whose double-hump long photometric cycle remains hitherto unexplained. We analyze photometric time series available in archive datasets sp…

astro-ph.GA2019★ 2 cited

Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1

D. Onić, M. D. Filipović, I. Bojičić +27

In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9+3.1. We present the radio spectral energy distr…