output
20042025
most citedA radio pulsing white dwarf binary star

215 citations

Showing 2016 · astro-ph.SRShow all

6 papers · 2 filters

astro-ph.SR2016★ 7 cited

An Investigation of Four Chemically Peculiar Stars with Photometric Periods below 12 Hours

Stefan Hümmerich, Klaus Bernhard, Ernst Paunzen +3

We present an investigation of three chemically peculiar (CP) stars and one CP star candidate which exhibit photometric periods below 12 hours. New spectroscopic observations have…

astro-ph.SR2016★ 40 cited

The beta Pictoris association: Catalog of photometric rotational periods of low-mass members and candidate members

S. Messina, M. Millward, A. Buccino +19

We intended to compile the most complete catalog of bona fide members and candidate members of the beta Pictoris association, and to measure their rotation periods and basic proper…

astro-ph.SR2016★ 21 cited

Return of the King: Time-Series Photometry of FO Aquarii's Initial Recovery from its Unprecedented 2016 Low State

Colin Littlefield, Peter Garnavich, Mark R. Kennedy +28

In 2016 May, the intermediate polar FO~Aqr was detected in a low state for the first time in its observational history. We report time-resolved photometry of the system during its…

astro-ph.SR2016★ 6 cited

The orbital ephemeris of the classical nova RR Pictoris: presence of a third body?

N. Vogt, M. R. Schreiber, F. -J. Hambsch +4

The ex-nova RR Pic presents a periodic hump in its light curve which is considered to refer to its orbital period. Analyzing all available epochs of these hump maxima in the litera…

astro-ph.SR2016★ 5 cited

NSV 1907 - A new eclipsing, nova-like cataclysmic variable

Stefan Hümmerich, Rainer Gröbel, Franz-Josef Hambsch +6

NSV 1907, formerly listed as an irregular variable in variability catalogues, was classified as an Algol-type eclipsing binary in the Catalina Surveys Periodic Variable Star Catalo…

astro-ph.SR2016★ 215 cited

A radio pulsing white dwarf binary star

T. R. Marsh, B. T. Gänsicke, S. Hümmerich +23

White dwarfs are compact stars, similar in size to Earth but ~200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengt…