The nearby SN 2017eaw is a Type II-P (" plateau") supernova (SN) showing early-time,
moderate CSM interaction. We present a comprehensive study of this SN, including the analysis …

Three of the seven rocky planets (e, f, and g) in TRAPPIST-1 system orbit in the habitable
zone of the host star. Therefore, water can be in liquid state at their surface being essential for …

The globular cluster Messier 80 was monitored by the Kepler space telescope for 80 days
during the K2 mission. Continuous, high-precision photometry of such an old, compact cluster …

One possible explanation of the cavity in debris discs is the gravitational perturbation of an
embedded giant planet. Planetesimals passing close to a massive body are dynamically …

Context. In the oligarchic growth model, protoplanets develop in the final stage of planet
formation via collisions between planetesimals and planetary embryos. The majority of …

Context. The modeling of stellar spectra of flux standards observed by the Hubble and
James Webb space telescopes requires a large synthetic spectral library that covers a wide …

After 25 years of the prediction of the possibility of observations, and despite the many hundreds
of well-studied transiting exoplanet systems, we are still waiting for the announcement …

Understanding the atmospheric parameters of stars on the top of the RGB is essential to
reveal the chemical composition of the Milky Way, as they can be used to probe the farthest …

… C virus in an oncology ward - Dencs - 2011 - Journal of Medical Virology - Wiley Online
Library … The authors thank Zoltán Kugler for his help in data collection and epidemiological …

We investigate the efficiency of moon formation around giant planets with numerical N-body
simulations and study the habitability of Earth-sized, newly formed moons. Our results show …