Zobrazeno 1 - 10
of 4 203
pro vyhledávání: '"WEISS, W"'
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:
Oplištilová, A., Mayer, P., Harmanec, P., Brož, M., Pigulski, A., Božić, H., Zasche, P., Šlechta, M., Pablo, H., Kołaczek-Szymański, P. A., Moffat, A. F. J., Lovekin, C. C., Wade, G. A., Zwintz, K., Popowicz, A., Weiss, W. W.
Publikováno v:
A&A 672, A31 (2023)
$\delta$ Orionis is the closest massive multiple stellar system and one of the brightest members of the Orion OB association. The primary (Aa1) is a unique evolved O star. In this work, we applied a two-step disentangling method to a series of spectr
Externí odkaz:
http://arxiv.org/abs/2301.10290
Autor:
Chopperla, Krishna Siva Teja, Kaladaran, Gopakumar, Kochaver, Anna K., Isgor, O. Burkan, Weiss, W. Jason
Publikováno v:
In Cement and Concrete Composites November 2024 154
Publikováno v:
In Cement June 2024 16
Autor:
W, Weiss W., K., Zwintz, R., Kuschnig, G., Handler, J., Moffat A. F., D., Baade, M., Bowman D., T., Granzer, T., Kallinger, F., Koudelka O., C., Lovekin C., C., Neiner, H., Pablo, A., Pigulski, A., Popowicz, T., Ramiaramanantsoa, M., Rucinski S., G., Strassmeier K., A, Wade G.
Publikováno v:
Universe 2021, 7, 199
BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and all
Externí odkaz:
http://arxiv.org/abs/2106.12952
Publikováno v:
In Construction and Building Materials 23 February 2024 417
Autor:
Kumar, Saurav, Imen, Sanaz, Sridharan, Vamsi Krishna, Gupta, Abhinav, McDonald, Walter, Ramirez-Avila, John J., Abdul-Aziz, Omar I., Talchabhadel, Rocky, Gao, Huilin, Quinn, Nigel W.T., Weiss, W. Josh, Poulose, Thomas, Palmate, Santosh S., Lee, Christine M., Baskaran, Latha
Publikováno v:
In Remote Sensing Applications: Society and Environment January 2024 33
Autor:
Weiss, W. W., Fröhlich, H. -E., Kallinger, T., Kuschnig, R., Popowicz, A., Baade, D., Buzasi, D., Handler, G., Kochukhov, O., Koudelka, O., Moffat, A. F. J., Pablo, B., Wade, G., Zwintz, K.
Publikováno v:
A&A 642, A64, 2020
Chemically peculiar (CP) stars with a measurable magnetic field comprise the group of mCP stars. The pulsating members define the subgroup of rapidly oscillating Ap (roAp) stars, of which Alpha Circini is the brightest member. Hence, Alpha Circini al
Externí odkaz:
http://arxiv.org/abs/2011.12597
Autor:
Beck, P. G., Kuschnig, R., Houdek, G., Kallinger, T., Weiss, W. W., Palle, P. L., Grundahl, F., Hatzes, A., Parviainen, H., Prieto, C. Allende, Deeg, H. J., Jiménez, A., Mathur, S., Garcia, R. A., White, T. R., Bedding, T. R., Grossmann, D. H., Janisch, S., Zaqarashvili, T., Hanslmeier, A., Zwintz, K., BRITE, the, teams, SONG
Solar-like oscillations in red-giant stars are now commonly detected in thousands of stars with space telescopes such as the NASA Kepler mission. Parallel radial velocity and photometric measurements would help to better understand the physics govern
Externí odkaz:
http://arxiv.org/abs/2001.04912
Autor:
Wade, G. A., Pigulski, A., Begy, S., Shultz, M., Handler, G., Sikora, J., Neilson, H., Cugier, H., Erba, C., Moffat, A. F. J., Pablo, B., Popowicz, A., Weiss, W., Zwintz, K.
Recent BRITE-Constellation space photometry of the slowly rotating, magnetic $\beta$ Cep pulsator $\xi^1$ CMa permits a new analysis of its pulsation properties. Analysis of the two-colour BRITE data reveals the well-known single pulsation period of
Externí odkaz:
http://arxiv.org/abs/1912.08347