activity
19972023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 4k across the 112 of their papers we have counts for

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Showing astro-ph.SRShow all

24 papers · 1 filter

astro-ph.SR2022★ 20 cited

The Galactic Nova Rate: Estimates from the ASAS-SN and Gaia Surveys

A. Kawash, L. Chomiuk, J. Strader +13

We present the first estimate of the Galactic nova rate based on optical transient surveys covering the entire sky. Using data from the All-Sky Automated Survey for Supernovae (ASA…

astro-ph.SR2022★ 8 cited

1RXH J082623.6-505741: a new long-period cataclysmic variable with an evolved donor and a low mass transfer rate

Kirill V. Sokolovsky, Jay Strader, Samuel J. Swihart +13

We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a K-t…

astro-ph.SR2022

Investigating the low-flux states in six Intermediate Polars

Ava E. Covington, Aarran W. Shaw, Koji Mukai +30

We present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr and RX J2133.7+5107, w…

astro-ph.SR2021

The 2019 outburst of the 2005 classical nova V1047 Cen: a record breaking dwarf nova outburst or a new phenomenon?

E. Aydi, K. V. Sokolovsky, J. S. Bright +28

We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years afte…

astro-ph.SR2020★ 28 cited

Increasing activity in T CrB suggests nova eruption is impending

Gerardo J. M. Luna, J. L. Sokoloski, K. Mukai +1

Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical expectations by orders of magnitude. This apparent discrepancy can be resolved if…

astro-ph.SR2020★ 21 cited

XMM-Newton observations of eleven intermediate polars and possible candidates

Hauke Wörpel, Axel Schwope, Iris Traulsen +2

We aim to identify new intermediate polars (IPs) in XMM-Newton observations from a list of promising candidates. By selecting targets not previously known to be X-ray bright we aim…