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20042018
most citedThe Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts

148 citations · 799 across the 22 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2017★ 25 cited

An UXor among FUors: extinction related brightness variations of the young eruptive star V582 Aur

P. Ábrahám, Á. Kóspál, M. Kun +24

V582 Aur is an FU Ori-type young eruptive star in outburst since 1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic va…

astro-ph.SR2017★ 28 cited

Photometric and radial-velocity time-series of RR Lyrae stars in M3: analysis of single-mode variables

J. Jurcsik, P. Smitola, G. Hajdu +18

We present the first simultaneous photometric and spectroscopic investigation of a large set of RR Lyrae variables in a globular cluster. The radial-velocity data presented compris…

astro-ph.SR2016★ 28 cited

The Continuing Story of SN IIb 2013df: New Optical and IR Observations and Analysis

Tamás Szalai, József Vinkó, Andrea P. Nagy +17

SN 2013df is a nearby Type IIb supernova that seems to be the spectroscopic twin of the well-known SN 1993J. Previous studies revealed many, but not all interesting properties of t…

astro-ph.SR2015★ 64 cited

Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

G. Dhungana, R. Kehoe, J. Vinko +32

We present extensive optical (, , and open CCD) and near-infrared () photometry for the very nearby Type IIP SN ~2013ej extending from +1 to +461 days after…

astro-ph.SR2015★ 49 cited

Overtone and multi-mode RR Lyrae stars in the globular cluster M3

J. Jurcsik, P. Smitola, G. Hajdu +15

The overtone and multi-mode RR Lyrae stars in the globular cluster M3 are studied using a 200-d long, and time-series photometry obtained in 2012. 70\% of the…

astro-ph.SR2013★ 33 cited

Exploring the circumstellar environment of the young eruptive star V2492 Cyg

Á. Kóspál, P. Ábrahám, J. A. Acosta-Pulido +20

Context. V2492 Cyg is a young eruptive star that went into outburst in 2010. The near-infrared color changes observed since the outburst peak suggest that the source belongs to a n…