Zobrazeno 1 - 10
of 2 428
pro vyhledávání: '"Budaj A"'
Publikováno v:
A&A 676, A88 (2023)
Spectra of planetary nebulae (PNe) are characterised by strong forbidden emission lines and often also by an infrared (IR) excess. A few PNe show dust obscuration events and/or harbour long-period binaries. Some post-asymptotic giant branch stars, sy
Externí odkaz:
http://arxiv.org/abs/2307.01331
Autor:
Krtička, J., Benáček, J., Budaj, J., Korčáková, D., Pál, A., Piecka, M., Zejda, M., Bakış, V., Brož, M., Chang, Hsiang-Kuang, Faltová, N., Gális, R., Jadlovský, D., Janík, J., Kára, J., Kolář, J., Krtičková, I., Kubát, J., Kubátová, B., Kurfürst, P., Labaj, M., Merc, J., Mikulášek, Z., Münz, F., Paunzen, E., Prišegen, M., Ramezani, T., Rievajová, T., Řípa, J., Schmidtobreick, L., Skarka, M., Szász, G., Weiss, W., Zajaček, M., Werner, N.
We outline the impact of a small two-band UV-photometry satellite mission on the field of stellar physics, magnetospheres of stars, binaries, stellar clusters, interstellar matter, and exoplanets. On specific examples of different types of stars and
Externí odkaz:
http://arxiv.org/abs/2306.15081
Autor:
Werner, N., Řípa, J., Münz, F., Hroch, F., Jelínek, M., Krtička, J., Zajaček, M., Topinka, M., Dániel, V., Gromeš, J., Václavík, J., Steiger, L., Lédl, V., Seginak, J., Benáček, J., Budaj, J., Faltová, N., Gális, R., Jadlovský, D., Janík, J., Kajan, M., Karas, V., Korčáková, D., Kosiba, M., Krtičková, I., Kubát, J., Kubátová, B., Kurfürst, P., Labaj, M., Mikulášek, Z., Pál, A., Paunzen, E., Piecka, M., Prišegen, M., Ramezani, T., Skarka, M., Szász, G., Thöne, C., Zejda, M.
We present a near-UV space telescope on a ~70kg micro-satellite with a moderately fast repointing capability and a near real-time alert communication system that has been proposed in response to a call for an ambitious Czech national mission. The mis
Externí odkaz:
http://arxiv.org/abs/2207.05485
Autor:
Vaňko, Martin, Pribulla, Theodor, Gajdoš, Pavol, Budaj, Ján, Zverko, Juraj, Paunzen, Ernst, Garai, Zoltán, Hambálek, Lubomír, Komžík, Richard, Kundra, Emil
There is a small group of peculiar early-type stars on the main sequence that show different rotation velocities from different spectral lines. This inconsistency might be due to the binary nature of these objects. We aim to verify this hypothesis by
Externí odkaz:
http://arxiv.org/abs/2204.03325
Publikováno v:
A&A, 660, A72 (2022)
WD 1145+017 is the first white dwarf known to be orbited by disintegrating exoasteroids. It is a DBZ-type white dwarf with strongly variable broad circumstellar lines and variable shallow UV transits. Various models of the dust clouds and gaseous rin
Externí odkaz:
http://arxiv.org/abs/2203.07520
Autor:
Bogumił Ramotowski, Anna Żuk, Paweł Lewandowski, Tomasz Słomski, Paweł Maciejewski, Andrzej Budaj
Publikováno v:
Advances in Interventional Cardiology, Vol 20, Iss 1, Pp 112-114 (2024)
Externí odkaz:
https://doaj.org/article/9015d94810c4446c8867f4d5a2e92a4a
Autor:
Zahger, Doron, Schwartz, Gregory G., Du, Weiming, Szarek, Michael, Bhatt, Deepak L., Bittner, Vera A., Budaj, Andrzej J., Diaz, Rafael, Goodman, Shaun G., Jukema, J. Wouter, Kiss, Robert G., Harrington, Robert A., Moriarty, Patrick M., Scemama, Michel, Manvelian, Garen, Pordy, Robert, White, Harvey D., Zeiher, Andreas M., Fazio, Sergio, Geba, Gregory P., Steg, Ph Gabriel
Publikováno v:
In Journal of the American College of Cardiology 10 September 2024 84(11):994-1006
Autor:
Vos, Joris, Pelisoli, Ingrid, Budaj, Jan, Reindl, Nicole, Schaffenroth, Veronika, Bobrick, Alexey, Geier, Stephan, Hermes, J. J., Nemeth, Peter, Østensen, Roy, Reding, Joshua S., Uzundag, Murat, Vuckovic, Maja
Publikováno v:
A&A 655, A43 (2021)
We present the discovery of J22564-5910, a new type of hot subdwarf (sdB) which shows evidence of gas present in the system and has shallow, multi-peaked hydrogen and helium lines which vary in shape over time. All observational evidence points towar
Externí odkaz:
http://arxiv.org/abs/2106.03363
Autor:
Budaj, Jan
Publikováno v:
Radiative Signatures from the Cosmos, ASP Conference Series, Vol. 519, p.87; 2019ASPC..519...87B
Program SHELLSPEC is designed to calculate light curves, spectra, and images of interacting binaries and extra-solar planets immersed in a moving gaseous or dusty circumstellar matter. It solves simple radiative transfer along the line of sight in 3D
Externí odkaz:
http://arxiv.org/abs/2105.00346
Autor:
Brož, M., Mourard, D., Budaj, J., Harmanec, P., Schmitt, H., Tallon-Bosc, I., Bonneau, D., Božić, H., Gies, D., Šlechta, M.
Publikováno v:
A&A 645, A51 (2021)
beta Lyr A is a complex binary system with an extensive observational dataset: light curves (from FUV to FIR), interferometric squared visibility, closure phase, triple product measurements, spectral-energy distribution (SED), high-resolution spectro
Externí odkaz:
http://arxiv.org/abs/2010.05541