Zobrazeno 1 - 10
of 32
pro vyhledávání: '"N. Themessl"'
Autor:
Andrés Jordán, Derek Buzasi, K. I. Collins, Joshua Pepper, Jon M. Jenkins, Alexander Lyttle, Martin Schlecker, Ismael Mireles, Sara Seager, Brett C. Addison, Andrea Miglio, Jack Okumura, Savita Mathur, Christopher Tylor, Daniel R. Hey, Victor Silva Aguirre, Zhao Guo, Tansu Daylan, Paula Sarkis, Mikkel N. Lund, J. S. Bentley, Martin Bo Nielsen, Joshua E. Schlieder, Keivan G. Stassun, Aldo Serenelli, Jonathan Horner, Stephen R. Kane, Tiago L. Campante, B. D. Carter, Joshua N. Winn, Hui Zhang, Diana Kossakowski, Thomas Henning, Brendan P. Bowler, Rasmus Handberg, Jake T. Clark, Warrick H. Ball, Matthew W. Mengel, Pamela Rowden, L. González-Cuesta, Karen A. Collins, Andrew W. Mann, Nicholas M. Law, John F. Kielkopf, B. Mosser, Daniel Huber, Ian J. M. Crossfield, Mathieu Clerte, Michaela Collins, Ashley Chontos, Songhu Wang, Belinda A. Nicholson, Pascal Torres, Thomas Kallinger, Robert A. Wittenmyer, Stephen C. Marsden, Andrew Vanderburg, Dag Evensberget, N. Themeßl, Rachel A. Matson, José Dias do Nascimento, David W. Latham, Cenk Kayhan, Timothy R. Bedding, Allen B. Davis, Emilie Laychock, J. O'Connor, Néstor Espinoza, B. Cale, Andrius Burnelis, S. Hekker, Steven D. Kawaler, Avi Shporer, Duncan J. Wright, Sarbani Basu, Peter Plavchan, James S. Kuszlewicz, Guy R. Davies, Teo Mocnik, Leandro de Almeida, Jason D. Eastman, Carl Ziegler, Rafael Brahm, Enrico Corsaro, William J. Chaplin, C. G. Tinney, Catherine Stevens, Rafael A. García, Sergi Blanco-Cuaresma, Steve B. Howell, Alexis Heitzmann, Roland Vanderspek, Thiam-Guan Tan, George R. Ricker
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Addison, B C, Wright, D J, Nicholson, B A, Cale, B, Mocnik, T, Huber, D, Plavchan, P, Wittenmyer, R A, Vanderburg, A, Chaplin, W J, Chontos, A, Clark, J T, Eastman, J D, Ziegler, C, Brahm, R, Carter, B D, Clerte, M, Espinoza, N, Horner, J, Bentley, J, Kane, S R, Kielkopf, J F, Laychock, E, Mengel, M W, Okumura, J, Stassun, K G, Bedding, T R, Bowler, B P, Burnelis, A, Collins, M, Crossfield, I, Davis, A B, Evensberget, D, Heitzmann, A, Howell, S B, Law, N, Mann, A W, Marsden, S, O'Connor, J, Shporer, A, Stevens, C, Tinney, C G, Tylor, C, Wang, S, Zhang, H, Henning, T, Kossakowski, D, Ricker, G, Sarkis, P, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Mireles, I, Rowden, P, Pepper, J, Daylan, T, Schlieder, J E, Collins, K A, Collins, K I, Tan, T-G, Ball, W H, Basu, S, Buzasi, D L, Campante, T L, Corsaro, E, González-Cuesta, L, Davies, G R, a, R A G, Guo, Z, Handberg, R, Hekker, S, Hey, D R, Kallinger, T, Kawaler, S D, Kayhan, C, Kuszlewicz, J S, Lund, M N, Lyttle, A, Mathur, S, Miglio, A, Mosser, B, Nielsen, M B, Serenelli, A M, Aguirre, V S & Themessl, N 2021, ' TOI-257b (HD 19916b) : a warm sub-saturn orbiting an evolved F-type star ', Monthly Notices of the Royal Astronomical Society, vol. 502, no. 3, pp. 3704-3722 . https://doi.org/10.1093/mnras/staa3960
arXiv
instname
Addison, B C, Wright, D J, Nicholson, B A, Cale, B, Mocnik, T, Huber, D, Plavchan, P, Wittenmyer, R A, Vanderburg, A, Chaplin, W J, Chontos, A, Clark, J T, Eastman, J D, Ziegler, C, Brahm, R, Carter, B D, Clerte, M, Espinoza, N, Horner, J, Bentley, J, Kane, S R, Kielkopf, J F, Laychock, E, Mengel, M W, Okumura, J, Stassun, K G, Bedding, T R, Bowler, B P, Burnelis, A, Collins, M, Crossfield, I, Davis, A B, Evensberget, D, Heitzmann, A, Howell, S B, Law, N, Mann, A W, Marsden, S, O'Connor, J, Shporer, A, Stevens, C, Tinney, C G, Tylor, C, Wang, S, Zhang, H, Henning, T, Kossakowski, D, Ricker, G, Sarkis, P, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Mireles, I, Rowden, P, Pepper, J, Daylan, T, Schlieder, J E, Collins, K A, Collins, K I, Tan, T-G, Ball, W H, Basu, S, Buzasi, D L, Campante, T L, Corsaro, E, González-Cuesta, L, Davies, G R, a, R A G, Guo, Z, Handberg, R, Hekker, S, Hey, D R, Kallinger, T, Kawaler, S D, Kayhan, C, Kuszlewicz, J S, Lund, M N, Lyttle, A, Mathur, S, Miglio, A, Mosser, B, Nielsen, M B, Serenelli, A M, Aguirre, V S & Themessl, N 2021, ' TOI-257b (HD 19916b) : a warm sub-saturn orbiting an evolved F-type star ', Monthly Notices of the Royal Astronomical Society, vol. 502, no. 3, pp. 3704-3722 . https://doi.org/10.1093/mnras/staa3960
arXiv
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3985bdf47299b8cd8d7592356769807c
Autor:
Alexey Mints, N. Themessl, Peter B. Stetson, J. De Ridder, Rafael A. García, Saskia Hekker, A. García Saravia Ortiz de Montellano
Publikováno v:
Themessl, N, Hekker, S, Mints, A, Garcia, R A, de Montellano, A G S O, Stetson, P B & De Ridder, J 2018, ' KIC 2568888 : To Be or Not to Be a Binary ', Astrophysical Journal, vol. 868, no. 2, 103 . https://doi.org/10.3847/1538-4357/aae846
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3868dee728d172db5c7f7c4b3b47bbc2
https://pure.au.dk/portal/da/publications/kic-2568888(9581ff20-1608-4264-9847-239832e2e4a8).html
https://pure.au.dk/portal/da/publications/kic-2568888(9581ff20-1608-4264-9847-239832e2e4a8).html
Publikováno v:
de Montellano, A G S O, Hekker, S & Themessl, N 2018, ' Automated asteroseismic peak detections ', Royal Astronomical Society. Monthly Notices, vol. 476, no. 2, pp. 1470-1496 . https://doi.org/10.1093/mnras/sty253
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12a2f44ff71d3a07de8e94bc9449d7b4
http://arxiv.org/abs/1801.09432
http://arxiv.org/abs/1801.09432
Autor:
Luca Fossati, Ehsan Moravveji, Norbert Przybilla, Konstanze Zwintz, Andrew Tkachenko, Victoria Antoci, Thomas G. Barnes, M.-F. Nieva, D. Lorenz, Rainer Kuschnig, Péter Pápics, N. Themessl
Publikováno v:
Zwintz, K, Moravveji, E, Papics, P I, Tkachenko, A, Przybilla, N, Nieva, M-F, Kuschnig, R, Antoci, V, Lorenz, D, Themessl, N, Fossati, L & Barnes, T G 2017, ' A comprehensive study of young B stars in NGC 2264 I. Space photometry and asteroseismology ', Astronomy & Astrophysics, vol. 601, 101 . https://doi.org/10.1051/0004-6361/201630327
Space photometric time series of the most massive members of the young open cluster NGC 2264 allow us to study their different sources of variability down to the millimagnitude level and permits a search for Slowly Pulsating B (SPB) type pulsation am
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b31eb8a05e455a0d890feda2ac2e593c
https://lirias.kuleuven.be/handle/123456789/590687
https://lirias.kuleuven.be/handle/123456789/590687
Akademický článek
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Autor:
Arlette Noels, M. A. G. Maia, Marie Martig, T. Morel, R. A. Garcia, Matthew Shetrone, Keivan G. Stassun, T. S. Rodrigues, Matthias Steinmetz, Sz. Meszaros, T. Kallinger, Paul Harding, Marica Valentini, Josefina Montalbán, D. P. Schneider, M. Schultheis, Friedrich Anders, J. A. Holtzman, R. de Assis Peralta, B. Mosser, S. Hekker, I. Minchev, L. N. da Costa, Andrea Miglio, C. Allende Prieto, Basilio X. Santiago, D. L. Nidever, N. Themeßl, S. R. Majewski, L. Girardi, S. Mathur, K. M. Cunha, F. Baudin, Cristina Chiappini, Timothy C. Beers, K. Pan, Ricardo P. Schiavon
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 576, pp.L12. ⟨10.1051/0004-6361/201525865⟩
Chiappini, C, Anders, F, Rodrigues, T S, Miglio, A, Montalban, J, Mosser, B, Girardi, L, Valentini, M, Noels, A, Morel, T, Minchev, I, Steinmetz, M, Santiago, B X, Schultheis, M, Martig, M, da Costa, L N, Maia, M A G, Allende Prieto, C, Peralta, R D A, Hekker, S, Themessl, N, Kallinger, T, Garcia, R A, Mathur, S, Baudin, F, Beers, T C, Cunhall, K, Harding, P, Holtzman, J, Majewski, S, Meszaros, S, Nidever, D, Pan, K, Schiavon, R P, Shetrone, M D, Schneider, D P & Stassun, K 2015, ' Young [α/Fe]-enhanced stars discovered by CoRoT and APOGEE : What is their origin? ', Astronomy & Astrophysics, vol. 576, L12 . https://doi.org/10.1051/0004-6361/201525865
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 576, pp.L12. ⟨10.1051/0004-6361/201525865⟩
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Astronomy and Astrophysics-A&A, 2015, 576, pp.L12. ⟨10.1051/0004-6361/201525865⟩
Chiappini, C, Anders, F, Rodrigues, T S, Miglio, A, Montalban, J, Mosser, B, Girardi, L, Valentini, M, Noels, A, Morel, T, Minchev, I, Steinmetz, M, Santiago, B X, Schultheis, M, Martig, M, da Costa, L N, Maia, M A G, Allende Prieto, C, Peralta, R D A, Hekker, S, Themessl, N, Kallinger, T, Garcia, R A, Mathur, S, Baudin, F, Beers, T C, Cunhall, K, Harding, P, Holtzman, J, Majewski, S, Meszaros, S, Nidever, D, Pan, K, Schiavon, R P, Shetrone, M D, Schneider, D P & Stassun, K 2015, ' Young [α/Fe]-enhanced stars discovered by CoRoT and APOGEE : What is their origin? ', Astronomy & Astrophysics, vol. 576, L12 . https://doi.org/10.1051/0004-6361/201525865
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 576, pp.L12. ⟨10.1051/0004-6361/201525865⟩
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
We report the discovery of a group of apparently young CoRoT red-giant stars exhibiting enhanced [alpha/Fe] abundance ratios (as determined from APOGEE spectra) with respect to Solar values. Their existence is not explained by standard chemical evolu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbe10e99bce452c24669f76684a2928e
http://arxiv.org/abs/1503.06990
http://arxiv.org/abs/1503.06990
Autor:
Paul G. Beck, N. Themessl, V. S. Schmid, R. E. Falcon, Péter Pápics, Michel Breger, V. Fritz, Conny Aerts, Jonas Debosscher, B. G. Castanheira
Publikováno v:
Astronomische Nachrichten. 333:1080-1082
Numerous high-resolution spectra of the δ Scuti star 4 CVn were gathered at McDonald Observatory in Texas, USA. They were prepared for interpretation using standard IRAF routines for a subsequent frequency analysis and mode identification with the s
Autor:
Jaymie M. Matthews, Slavek M. Rucinski, Luca Fossati, A. F. J. Moffat, S. Pollack-Drs, Dimitar Sasselov, Konstanze Zwintz, T. A. Ryabchikova, Werner W. Weiss, A. Baglin, N. Themeßl, Ehsan Moravveji, M. Rainer, David B. Guenther, Conny Aerts, E. Poretti, D. Lorenz, Thomas G. Barnes, C. Cameron, Rainer Kuschnig
Publikováno v:
Science
Science, American Association for the Advancement of Science, 2014, 345 (6196), pp.550-553. ⟨10.1126/science.1253645⟩
Science, 2014, 345 (6196), pp.550-553. ⟨10.1126/science.1253645⟩
Science, 345, 6196, pp. 550-553
Science, 345, 550-553
Science, American Association for the Advancement of Science, 2014, 345 (6196), pp.550-553. ⟨10.1126/science.1253645⟩
Science, 2014, 345 (6196), pp.550-553. ⟨10.1126/science.1253645⟩
Science, 345, 6196, pp. 550-553
Science, 345, 550-553
We demonstrate that a seismic analysis of stars in their earliest evolutionary phases is a powerful method to identify young stars and distinguish their evolutionary states. The early star that is born from the gravitational collapse of a molecular c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9132e5cb3537295bc6e53a83161227f
https://hal.archives-ouvertes.fr/hal-02551205
https://hal.archives-ouvertes.fr/hal-02551205
Autor:
K, Zwintz, L, Fossati, T, Ryabchikova, D, Guenther, C, Aerts, T G, Barnes, N, Themeßl, D, Lorenz, C, Cameron, R, Kuschnig, S, Pollack-Drs, E, Moravveji, A, Baglin, J M, Matthews, A F J, Moffat, E, Poretti, M, Rainer, S M, Rucinski, D, Sasselov, W W, Weiss
Publikováno v:
Science (New York, N.Y.). 345(6196)
We demonstrate that a seismic analysis of stars in their earliest evolutionary phases is a powerful method with which to identify young stars and distinguish their evolutionary states. The early star that is born from the gravitational collapse of a
Autor:
Slavek M. Rucinski, Dimitar Sasselov, David B. Guenther, A. F. J. Moffat, Luca Fossati, Werner W. Weiss, A. Baglin, M. Auvergne, K. Zwintz, N. Themessl, Rainer Kuschnig, J. M. Matthews, S. Chaintreuil, Jason F. Rowe, T. A. Ryabchikova, D. A. Bohlender, Thomas G. Barnes
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 552, pp.A68. ⟨10.1051/0004-6361/201220934⟩
Astronomy and Astrophysics-A&A, 2013, 552, pp.A68. ⟨10.1051/0004-6361/201220934⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2013, 552, pp.A68. ⟨10.1051/0004-6361/201220934⟩
Astronomy and Astrophysics-A&A, 2013, 552, pp.A68. ⟨10.1051/0004-6361/201220934⟩
We concentrate on an asteroseismological study of HD 261711, a rather hot delta Scuti type pulsating member of the young open cluster NGC 2264 located at the blue border of the instability region. HD 261711 was discovered to be a pre-main sequence de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9848f5afbd6739580b5bba02dfe137c5
https://hal.archives-ouvertes.fr/hal-02524358
https://hal.archives-ouvertes.fr/hal-02524358