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20182023
most citedA low-luminosity core-collapse supernova very similar to SN 2005cs

14 citations · 38 across the 5 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR2023

Detailed asteroseismic modeling of RR Lyrae stars with non-radial modes

H. Netzel, L. Molnar, M. Joyce

Photometric observations from the last decade have revealed additional low-amplitude periodicities in many classical pulsators that are likely due to pulsations in non-radial modes…

astro-ph.SR20238 cited

Comment on the feasibility of carbon burning in Betelgeuse: a response to "The evolutionary stage of Betelgeuse inferred from its pulsation periods," arXiv:2306.00287

László Molnár, Meridith Joyce, Shing-Chi Leung

The recent pre-print by Saio et al. 2023 argues that the supergiant Betelgeuse is already undergoing carbon burning, based on the assumption that all of its light variations are ca…

astro-ph.SR2023

Frequency analysis of the first-overtone RR Lyrae stars based on the Extended Aperture Photometry from the K2 data

H. Netzel, L. Molnar, E. Plachy +1

Additional low-amplitude signals are observed in many RR Lyrae stars, beside the pulsations in radial modes. The most common ones are short-period signals forming a period ratio of…

astro-ph.SR202111 cited

HD344787: a true Polaris analogue?

V. Ripepi, G. Catanzaro, L. Molnár +10

Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic distance scale, but they are also important objects per se, allowing us to put constraint…

astro-ph.SR202014 cited

A low-luminosity core-collapse supernova very similar to SN 2005cs

Zoltán Jäger, József Vinkó, Barna I. Bíró +5

We present observations and analysis of PSN J17292918+7542390, a low-luminosity Type II-P supernova (LL SN IIP). The observed sample of such events is still low, and their nature i…

astro-ph.SR20205 cited

X-ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-Mass Companion

Nancy Remage Evans, Ignazio Pillitteri, Laszlo Molnar +17

V473 Lyr is a classical Cepheid which is unique in having substantial amplitude variations with a period of approximately 3.3 years, thought to be similar to the Blazhko variations…