Zobrazeno 1 - 10
of 454
pro vyhledávání: '"Karczmarek P"'
Autor:
García, G. Rojas, Graczyk, D., Pietrzyński, G., Gałan, C., Gieren, W., Thompson, I., Suchomska, K., Kałuszyński, M., Soszyński, I., Udalski, A., Karczmarek, P., Narloch, W., Górski, M., Wielgórski, P., Zgirski, B., Miller, N., Hajdu, G., Pilecki, B., Taormina, M., Lewis, M.
Publikováno v:
A&A 692, A110 (2024)
Detached eclipsing binaries (DEBs) allow for the possibility of precise characterization of its stellar components. They offer a unique opportunity to derive their physical parameters in a near-model-independent way for a number of systems consisting
Externí odkaz:
http://arxiv.org/abs/2410.18619
Autor:
Wielgórski, Piotr, Pietrzyński, Grzegorz, Gieren, Wolfgang, Zgirski, Bartłomiej, Górski, Marek, Storm, Jesper, Nardetto, Nicolas, Kervella, Pierre, Bras, Garance, Hajdu, Gergely, Hocdé, Vincent, Pilecki, Bogumił, Narloch, Weronika, Karczmarek, Paulina, Pych, Wojciech, Chini, Rolf, Hodapp, Klaus
Type II Cepheids are old pulsating stars that can be used to trace the distribution of an old stellar population and to measure distances to globular clusters and galaxies within several megaparsecs. One method that can be used to measure the distanc
Externí odkaz:
http://arxiv.org/abs/2406.16561
Autor:
Narloch, W., Hajdu, G., Pietrzynski, G., Gieren, W., Zgirski, B., Wielgorski, P., Karczmarek, P., Gorski, M., Graczyk, D.
RR Lyrae stars are excellent tracers of the old population II due to their period-luminosity (PL) and period-luminosity-metallicity (PLZ) relations. While these relations have been investigated in detail in many photometric bands, there are few compr
Externí odkaz:
http://arxiv.org/abs/2406.12408
Autor:
Rathour, Rajeev Singh, Hajdu, Gergely, Smolec, Radosław, Karczmarek, Paulina, Hocdé, Vincent, Ziółkowska, Oliwia, Soszyński, Igor, Udalski, Andrzej
Publikováno v:
A&A 686, A268 (2024)
Period change studies give a window to probe into the evolution and dynamics of Cepheids. While evolutionary period changes have been well studied both observationally and theoretically, non-evolutionary period changes lack a systematic and quantitat
Externí odkaz:
http://arxiv.org/abs/2403.14039
Autor:
Pilecki, Bogumił, Thompson, Ian B., Espinoza-Arancibia, Felipe, Hajdu, Gergely, Gieren, Wolfgang, Taormina, Mónica, Pietrzyński, Grzegorz, Narloch, Weronika, Bono, Giuseppe, Gallenne, Alexandre, Kervella, Pierre, Wielgórski, Piotr, Zgirski, Bartłomiej, Graczyk, Dariusz, Karczmarek, Paulina, Evans, Nancy R.
Publikováno v:
A&A 686, A263 (2024)
Binary Cepheids with giant companions are crucial for studying the physical properties of Cepheid variables, providing the best means to measure their masses. Systems composed of two Cepheids are even more important but to date, only one such system
Externí odkaz:
http://arxiv.org/abs/2403.12390
Autor:
Lewis, M. O., Bhattacharya, R., Sjouwerman, L. O., Pihlström, Y. M., Pietrzyński, G., Sahai, R., Karczmarek, P., Górski, M.
Publikováno v:
A&A 677, A153 (2023)
We establish a sample of 370 Mira variables that are likely near the Galactic center (GC). The sources have been selected from the OGLE and BAaDE surveys based on their sky coordinates, OGLE classifications, and BAaDE maser-derived line-of-sight velo
Externí odkaz:
http://arxiv.org/abs/2308.01710
Autor:
Narloch, Weronika, Hajdu, Gergely, Pietrzynski, Grzegorz, Gieren, Wolfgang, Wielgorski, Piotr, Zgirski, Bartlomiej, Karczmarek, Paulina, Gorski, Marek, Graczyk, Dariusz
We present the first period-luminosity (PL) and period-Wesenheit (PW) relations in the Sloan-Pans-STARRS gP1rP1iP1 bands for classical fundamental mode Cepheids in the Milky Way. We used a relatively modest number of 76 stars for the PL and 84-85 sta
Externí odkaz:
http://arxiv.org/abs/2306.06326
Autor:
Project, The Araucaria, Pietrzyński, G., Gieren, W., Karczmarek, P., Górski, M., Zgirski, B., Wielgórski, P., Breuval, L., Suchomska, K., Gallenne, A., Kervella, P., Hajdu, G., Pilecki, B., Storm, J., Nardetto, N., Kudritzki, R. P., Taormina, M., Bresolin, F., Smolec, R., Narloch, W., Gałan, C., Lewis, M., Chini, R.
Publikováno v:
Published on behalf of the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences. Editors: P. Karczmarek, M. Lewis, G. Pietrzy\'nski. Publisher: Wydawnictwo Aleksander, Pu{\l}tusk 2021. ISBN: 978-83-66856-07-3
The book consists of a number of short articles that present achievements of the Araucaria members, collaborators, and friends, in various aspects of distance determinations and related topics. It celebrates the 20-year anniversary of the Araucaria P
Externí odkaz:
http://arxiv.org/abs/2305.17247
Autor:
Zgirski, Bartłomiej, Pietrzyński, Grzegorz, Górski, Marek, Gieren, Wolfgang, Wielgórski, Piotr, Karczmarek, Paulina, Hajdu, Gergely, Lewis, Megan, Chini, Rolf, Graczyk, Dariusz, Kałuszyński, Mikołaj, Narloch, Weronika, Pilecki, Bogumił, García, Gonzalo Rojas, Suchomska, Ksenia, Taormina, Mónica
We present new period-luminosity and period-luminosity-metallicity relations for Galactic RR Lyrae stars based on a sample of 28 pulsators located at distances up to $1.5$ kpc from the Sun. Near-infrared photometry was obtained at the Cerro Armazones
Externí odkaz:
http://arxiv.org/abs/2305.09414
Autor:
Karczmarek, Paulina, Hajdu, Gergely, Pietrzyński, Grzegorz, Gieren, Wolfgang, Narloch, Weronika, Smolec, Radosław, Wiktorowicz, Grzegorz, Belczynski, Krzysztof
Because of their period-luminosity relation (PLR), classical Cepheids play a key role in the calibration of the extragalactic distance scale and the determination of the Hubble-Lema\^{i}tre constant $H_0$. Recent findings show that the majority of cl
Externí odkaz:
http://arxiv.org/abs/2303.15664