activity
20142016
most citedA radio pulsing white dwarf binary star

215 citations · 238 across the 9 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.SR20167 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

A New Sample of Mid-Infrared Bright, Long-Period Mira Variables from the MACHO Galactic Bulge Fields

Klaus Bernhard, Stefan Uttenthaler, Stefan Hümmerich

Mid-infrared bright objects in the direction of the Galactic Bulge were investigated using time series photometry from the MACHO data archive, which led to the discovery of a large…

astro-ph.SR2016

An investigation of the RCB star candidate GDS J0702414-023501

Stefan Huemmerich, Klaus Bernhard

2MASS J07024146-0235017 = GDS J0702414-023501 was included in the "Catalogue enriched with R CrB stars" on grounds of its near- and mid-infrared colours. The object, which correspo…

astro-ph.SR201610 cited

HD 240121 - an ACV variable showing anti-phase variations of the B and V light curves

Rainer Gröbel, Stefan Hümmerich, Ernst Paunzen +1

The variability of HD 240121 = BD+59 2602 was first suspected by Särg & Wramdemark (1970) and later confirmed by Gröbel (1992a,b). Because of the observed anti-phase variations of…

astro-ph.SR20165 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.SR2016215 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…