activity
20122017
most citedAn unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova

94 citations · 94 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2017

Atomic diffusion in the atmosphere of Feige 86

Peter Nemeth

We have revisited the ultraviolet and optical spectra of the blue horizontal branch star Feige 86. The new analysis finds the star cooler and more compact than previously determine…

astro-ph.IM2017

Astroserver - Research Services in the Stellar Webshop

Peter Nemeth

A quick look at research and development in astronomy shows that we live in exciting times. Exoplanetary systems, supernovae, and merging binary black holes were far out of reach f…

astro-ph.SR2017

A FEROS Survey of Hot Subdwarf Stars

S. Vennes, P. Nemeth, A. Kawka

We have completed a survey of twenty-two ultraviolet-selected hot subdwarfs using the Fiber-fed Extended Range Optical Spectrograph (FEROS) and the 2.2-m telescope at La Silla. The…

astro-ph.SR2017

Meet the family - the catalog of known hot subdwarf stars

Stephan Geier, Roy H. Østensen, Peter Nemeth +6

In preparation for the upcoming all-sky data releases of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpubl…

astro-ph.SR201794 cited

An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova

S. Vennes, P. Nemeth, A. Kawka +4

Subluminous Type Ia supernovae, such as the Type Iax class prototype SN 2002cx, are described by a variety of models such as the failed detonation and partial deflagration of an ac…

astro-ph.SR2013

Non-LTE Luminosity and Abundance Diagnostics of Classical Novae in X-rays

Péter Németh

Classical novae are significant sources of interstellar material, especially carbon, nitrogen and oxygen. These standard candles are only behind supernovae and -ray bursts as th…