Showing 1–20 of 79 results
/ Date/ Name
Jun 9, 2023Comment on the feasibility of carbon burning in Betelgeuse: a response to "The evolutionary stage of Betelgeuse inferred from its pulsation periods," arXiv:2306.00287Feb 14, 2023Educated towards research: the first five years of the undergraduate mentoring program at Konkoly ObservatoryMay 29, 2018Gaia Data Release 2: Validation of the classification of RR Lyrae and Cepheid variables with the Kepler and K2 missionsOct 6, 2016Variable stars with the Kepler space telescopeJun 21, 2023Asteroseismic sounding of bulge globular clusters with the Roman Space TelescopeFeb 2, 2016The first decade of RR Lyrae space photometric observationsJun 16, 2020Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESAAug 3, 2023To Grow Old and Peculiar: A Survey of Anomalous Variable Stars in M80 and Age Determination using K2 and GaiaJun 2, 2014V473 Lyrae, a unique second-overtone Cepheid with two modulation cyclesMay 26, 2025Asteroseismic mass and radius of the naked-eye red giant HD145250Sep 15, 2021First results on RR Lyrae stars with the TESS space telescope: untangling the connections between mode content, colors and distancesMay 2, 2019Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae MinorisNov 11, 2022Type II and anomalous Cepheids in the Kepler K2 missionSep 9, 2024Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4Jan 18, 2020Rotational properties of Hilda asteroids observed by the K2 missionMar 28, 2018Shockwave Behaviour in RR Lyrae StarsMar 9, 2016Large size and slow rotation of the trans-Neptunian object (225088) 2007 OR10 discovered from Herschel and K2 observationsMar 1, 2025Filling the gap: the missing eclipses of $γ$ Persei from 2005 and from 2006Mar 2, 2025Search for binary-channel metal-rich RR~Lyrae candidatesDec 12, 2024A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC