134 citations
- Á. Kóspál2 profiles26 · h 31
- P. Ábrahám3 profiles16 · h 22
- M. Pignatari2 profiles11 · h 42
- M. Lugaro8 · h 42
- Fernando Cruz-Sáenz de Miera7
- A. P'al2 profiles6 · h 21
- B. Nisini2 profiles6 · h 44
- L. Kriskovics2 profiles6 · h 20
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- A. Moór2 profiles5 · h 21
- B. Cseh5 · h 15
- E. Plachy2 profiles5 · h 29
- Konkoly ObservatoryHU76 papers
- HUN-REN Research Centre for Astronomy and Earth SciencesHU70 papers
- Eötvös Loránd UniversityHU53 papers
- Max Planck Institute for AstronomyDE34 papers
- Centre National de la Recherche ScientifiqueFR21 papers
- European Southern ObservatoryCL17 papers
- Monash UniversityAU14 papers
- Astronomical Observatory of CapodimonteIT11 papers
- Astronomical Observatory of RomeIT10 papers
- Institut de Planétologie et d'Astrophysique de GrenobleFR10 papers
- Space Telescope Science InstituteUS10 papers
- Université Grenoble AlpesFR10 papers
28 papers · 1 filter
High-resolution spectroscopic analysis of four new chemically peculiar stars
M. P. Roriz, C. B. Pereira, S. Junqueira +3
We present detailed chemical compositions of four stars on the first-ascent red giant branch that are classified as chemically peculiar, but lack comprehensive analyses at high spe…
Type II and anomalous Cepheids in the Kepler K2 mission
Monika I. Jurkovic, Emese Plachy, László Molnár +4
We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kepler K2 mission. The precise light curves of these pulsating variable stars are t…
Accretion process, magnetic fields, and apsidal motion in the pre-main sequence binary DQ Tau
Kim Pouilly, Oleg Kochukhov, Ágnes Kóspál +3
Classical T Tauri stars (CTTSs) are young stellar objects that accrete materials from their accretion disc influenced by their strong magnetic field. The magnetic pressure truncate…
Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1
A. Moór, P. Ábrahám, Á. Kóspál +23
Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and…
Deep underground laboratory measurement of C(,)O in the Gamow windows of the - and -processes
B. Gao, T. Y. Jiao, Y. T. Li +71
The C(,)O reaction is the main neutron source for the slow-neutron-capture (s-) process in Asymptotic Giant Branch stars and for the intermediate (i-) process.…
The relation between the Mass Accretion Rate and the Disk Mass in Class I Protostars
Eleonora Fiorellino, Lukasz Tychoniec, Carlo F. Manara +5
The evidence of a relation between the mass accretion rate and the disk mass is established for young, Class II pre-main sequence stars. This observational result opened an avenue…