activity
19992014
most citedDust formation in the ejecta of the Type II-P supernova 2004dj

66 citations · 383 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2014★ 5 cited

Discovery of the spectroscopic binary nature of the classical Cepheids FN Aql and V1344 Aql

L. Szabados, B. Cseh, J. Kovács +8

We present the analysis of photometric and spectroscopic data of two classical Cepheids, FN Aquilae and V1344 Aquilae. Based on the joint treatment of the new and earlier radial ve…

astro-ph.SR2010★ 66 cited

Dust formation in the ejecta of the Type II-P supernova 2004dj

T. Szalai, J. Vinkó, Z. Balog +3

Core-collapse supernovae (CC SNe), especially Type II-Plateau ones, are thought to be important contributors to cosmic dust production. SN 2004dj, one of the closest and brightest…

astro-ph2008★ 52 cited

The Young, Massive, Star Cluster Sandage-96 After the Explosion of SN 2004dj in NGC 2403

J. Vinko, K. Sarneczky, Z. Balog +12

The bright Type II-plateau supernova (SN) 2004dj occurred within the young, massive stellar cluster Sandage-96 in a spiral arm of NGC 2403. New multi-wavelength observations obtain…

astro-ph2005

A comprehensive survey of variable stars in the globular cluster NGC 362

P. Székely, L. L. Kiss, B. Csák +3

We present the first results of our variability survey for the globular cluster NGC 362. We found numerous variable stars in the field including 23 RR Lyr stars, 4 eclipsing binari…

astro-ph2004★ 26 cited

Spectroscopic monitoring of the transition phase in nova V4745 Sgr

B. Csak, L. L. Kiss, A. Retter +2

We present a spectroscopic monitoring of the transient nova V4745 Sagittarii (Nova Sgr 2003 #1) covering ten months after the discovery. During this period the light curve showed w…

astro-ph2002★ 17 cited

The He-shell flash in action: T Ursae Minoris revisited

K. Szatmary, L. L. Kiss, Zs. Bebesi

We present an updated and improved description of the light curve behaviour of T Ursae Minoris, which is a Mira star with the strongest period change (the present rate is an amazin…