Zobrazeno 1 - 10
of 384
pro vyhledávání: '"Themessl A"'
Context. Stars that are members of stellar clusters are assumed to be formed at the same time and place from material with the same initial chemical composition. These additional constraints on the ensemble of cluster stars make these stars suitable
Externí odkaz:
http://arxiv.org/abs/2310.06757
Autor:
Yu, Jie, Khanna, Shourya, Themessl, Nathalie, Hekker, Saskia, Dréau, Guillaume, Gizon, Laurent, Bi, Shaolan
Asteroseismology has become widely accepted as a benchmark for accurate and precise fundamental stellar properties. It can therefore be used to validate and calibrate stellar parameters derived from other approaches. Meanwhile, one can leverage large
Externí odkaz:
http://arxiv.org/abs/2206.00046
Autor:
Addison, Brett C., Wright, Duncan J., Nicholson, Belinda A., Cale, Bryson, Mocnik, Teo, Huber, Daniel, Plavchan, Peter, Wittenmyer, Robert A., Vanderburg, Andrew, Chaplin, William J., Chontos, Ashley, Clark, Jake T., Eastman, Jason D., Ziegler, Carl, Brahm, Rafael, Carter, Bradley D., Clerte, Mathieu, Espinoza, Néstor, Horner, Jonathan, Bentley, John, Jordán, Andrés, Kane, Stephen R., Kielkopf, John F., Laychock, Emilie, Mengel, Matthew W., Okumura, Jack, Stassun, Keivan G., Bedding, Timothy R., Bowler, Brendan P., Burnelis, Andrius, Blanco-Cuaresma, Sergi, Collins, Michaela, Crossfield, Ian, Davis, Allen B., Evensberget, Dag, Heitzmann, Alexis, Howell, Steve B., Law, Nicholas, Mann, Andrew W., Marsden, Stephen C., Matson, Rachel A., O'Connor, James, Shporer, Avi, Stevens, Catherine, Tinney, C. G., Tylor, Christopher, Wang, Songhu, Zhang, Hui, Henning, Thomas, Kossakowski, Diana, Ricker, George, Sarkis, Paula, Schlecker, Martin, Torres, Pascal, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Mireles, Ismael, Rowden, Pam, Pepper, Joshua, Daylan, Tansu, Schlieder, Joshua E., Collins, Karen A., Collins, Kevin I., Tan, Thiam-Guan, Ball, Warrick H., Basu, Sarbani, Buzasi, Derek L., Campante, Tiago L., Corsaro, Enrico, González-Cuesta, Lucía, Davies, Guy R., de Almeida, Leandro, Nascimento, Jr., Jose-Dias do, a, Rafael A. Garcí, Guo, Zhao, Handberg, Rasmus, Hekker, Saskia, Hey, Daniel R., Kallinger, Thomas, Kawaler, Steven D., Kayhan, Cenk, Kuszlewicz, James S., Lund, Mikkel N., Lyttle, Alexander, Mathur, Savita, Miglio, Andrea, Mosser, Benoit, Nielsen, Martin B., Serenelli, Aldo M., Aguirre, Victor Silva, Themeßl, Nathalie
We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS and confirmed to be of planetary origin based on radial velocity obser
Externí odkaz:
http://arxiv.org/abs/2001.07345
Autor:
Chaplin, William J., Serenelli, Aldo M., Miglio, Andrea, Morel, Thierry, Mackereth, J. Ted, Vincenzo, Fiorenzo, Basu, Hans Kjeldsen Sarbani, Ball, Warrick H., Stokholm, Amalie, Verma, Kuldeep, Mosumgaard, Jakob Rørsted, Aguirre, Victor Silva, Mazumdar, Anwesh, Ranadive, Pritesh, Antia, H. M., Lebreton, Yveline, Ong, Joel, Appourchaux, Thierry, Bedding, Timothy R., Christensen-Dalsgaard, Jørgen, Creevey, Orlagh, García, Rafael A., Handberg, Rasmus, Huber, Daniel, Kawaler, Steven D., Lund, Mikkel N., Metcalfe, Travis S., Stassun, Keivan G., Bazot, Michäel, Beck, Paul, Bell, Keaton J., Bergemann, Maria, Buzasi, Derek L., Benomar, Othman, Bossini, Diego, Bugnet, Lisa, Campante, Tiago L., Orhan, Zeynep Çelik, Corsaro, Enrico, González-Cuesta, Lucía, Davies, Guy R., Di Mauro, Maria Pia, Egeland, Ricky, Elsworth, Yvonne P., Gaulme, Patrick, Ghasemi, Hamed, Guo, Zhao, Hall, Oliver J., Hasanzadeh, Amir, Hekker, Saskia, Howe, Rachel, Jenkins, Jon M., Jiménez, Antonio, Kiefer, René, Kuszlewicz, James S., Kallinger, Thomas, Latham, David W., Lundkvist, Mia S., Mathur, Savita, Montalbán, Josefina, Mosser, Benoit, Bedón, Andres Moya, Nielsen, Martin Bo, Örtel, Sibel, Rendle, Ben M., Ricker, George R., Rodrigues, Thaíse S., Roxburgh, Ian W., Safari, Hossein, Schofield, Mathew, Seager, Sara, Smalley, Barry, Stello, Dennis, Szabó, Róbert, Tayar, Jamie, Themeßl, Nathalie, Thomas, Alexandra E. L., Vanderspek, Roland K., van Rossem, Walter E., Vrard, Mathieu, Weiss, Achim, White, Timothy R., Winn, Joshua N., Yıldız, Mutlu
Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. While these accreted stellar populations can be forensically identified as kinematically distinct structures within the Galaxy, it is difficult in general
Externí odkaz:
http://arxiv.org/abs/2001.04653
Autor:
Alexander Themessl, Timon Wagner, Marco-Christopher Rupp, Hannes Degenhardt, Klaus Woertler, Kate A. Hatter, Andreas B. Imhoff, Sebastian Siebenlist, Jonas Pogorzelski
Publikováno v:
BMC Musculoskeletal Disorders, Vol 24, Iss 1, Pp 1-8 (2023)
Abstract Background Rotator cuff tears among patients under 50 years either result from an adequate trauma or are considered non-traumatic due to work-related or athletic overuse. The impact of these different mechanisms on postoperative functional o
Externí odkaz:
https://doaj.org/article/eb8b311607ea4470922e7a373199bf67
Autor:
Themeßl, N., Hekker, S., Mints, A., García, R. A., de Montellano, A. García Saravia Ortiz, Stetson, P. B., De Ridder, J.
In cases where both components of a binary system show oscillations, asteroseismology has been proposed as a method to identify the system. For KIC 2568888, observed with $Kepler$, we detect oscillation modes for two red giants in a single power dens
Externí odkaz:
http://arxiv.org/abs/1810.06206
Autor:
Themeßl, N., Hekker, S., Southworth, J., Beck, P. G., Pavlovski, K., Tkachenko, A., Angelou, G. C., Ball, W. H., Barban, C., Corsaro, E., Elsworth, Y., Handberg, R., Kallinger, T.
The internal structures and properties of oscillating red-giant stars can be accurately inferred through their global oscillation modes (asteroseismology). Based on 1460 days of Kepler observations we perform a thorough asteroseismic study to probe t
Externí odkaz:
http://arxiv.org/abs/1804.11151
Individual mode frequencies have been detected in thousands of individual solar-like oscillators on the red giant branch (RGB). Fitting stellar models to these mode frequencies, however, is more difficult than in main-sequence stars. This is partly b
Externí odkaz:
http://arxiv.org/abs/1804.11153
Space observatories such as $\textit{Kepler}$ have provided data that can potentially revolutionise our understanding of stars. Through detailed asteroseismic analyses we are capable of determining fundamental stellar parameters and reveal the stella
Externí odkaz:
http://arxiv.org/abs/1801.09432
Autor:
Rupp, Marco-Christopher, Muench, Lukas N., Ehmann, Yannick J., Themessl, Alexander, Winkler, Philipp W., Mehl, Julian, Imhoff, Andreas B., Feucht, Matthias J.
Publikováno v:
In Arthroscopy: The Journal of Arthroscopic and Related Surgery June 2022 38(6):1944-1953