Zobrazeno 1 - 10
of 178
pro vyhledávání: '"Bell, Keaton J."'
Autor:
Calcaferro, Leila M., Sowicka, Paulina, Uzundag, Murat, Córsico, Alejandro H., Kepler, S. O., Bell, Keaton J., Althaus, Leandro G., Handler, Gerald, Kawaler, Steven D., Werner, Klaus
Publikováno v:
A&A 686, A140 (2024)
Significant advances have been achieved through the latest improvements in the photometric observations accomplished by the recent space missions, substantially boosting the study of pulsating stars via asteroseismology. The TESS mission has already
Externí odkaz:
http://arxiv.org/abs/2402.16642
Autor:
Hernandez, Mercedes S., Schreiber, Matthias R., Landstreet, John D., Bagnulo, Stefano, Parsons, Steven G., Chavarria, Martin, Toloza, Odette, Bell, Keaton J.
Recent surveys of close white dwarf binaries as well as single white dwarfs have provided evidence for the late appearance of magnetic fields in white dwarfs, and a possible generation mechanism a crystallization and rotation-driven dynamo has been s
Externí odkaz:
http://arxiv.org/abs/2401.15158
Autor:
Uzundag, Murat, De Gerónimo, Francisco C., Córsico, Alejandro H., Silvotti, Roberto, Bradley, Paul A., Montgomery, Michael H., Catelan, Márcio, Toloza, Odette, Bell, Keaton J., Kepler, S. O., Althaus, Leandro G., Kleinman, Scot J., Kilic, Mukremin, Mullally, Susan E., Gänsicke, Boris T., Bąkowska, Karolina, Barber, Sam, Nitta, Atsuko
G\,29$-$38 (TIC~422526868) is one of the brightest ($V=13.1$) and closest ($d = 17.51$\,pc) pulsating white dwarfs with a hydrogen-rich atmosphere (DAV/ZZ Ceti class). It was observed by the {\sl TESS} spacecraft in sectors 42 and 56. The atmosphere
Externí odkaz:
http://arxiv.org/abs/2309.04809
Frymire & Ardila (2023) reported an anomalous flux variation in the Transiting Exoplanet Survey Satellite (TESS) Sector 43 light curve of the white dwarf HZ 4. We show that this flux variation was caused by the main-belt asteroid 4382 Stravinsky trav
Externí odkaz:
http://arxiv.org/abs/2307.15085
Autor:
Pedersen, May G., Bell, Keaton J.
Given its large plate scale of 21" / pixel, analyses of data from the TESS space telescope must be wary of source confusion from blended light curves, which creates the potential to attribute observed photometric variability to the wrong astrophysica
Externí odkaz:
http://arxiv.org/abs/2304.05706
Autor:
Romero, Alejandra D., da Rosa, Gabriela Oliveira, Kepler, S. O., Bradley, Paul A., Uzundag, Murat, Bell, Keaton J., Hermes, J. J., Lauffer, G. R.
We present the photometric data from TESS for two known ZZ Ceti stars, PG 1541+651 and BPM 31594. Before TESS, both objects only had observations from short runs from ground-based facilities, with three and one period detected, respectively. The TESS
Externí odkaz:
http://arxiv.org/abs/2210.15163
Autor:
Córsico, Alejandro H., Uzundag, Murat, Kepler, S. O., Althaus, Leandro G., Silvotti, Roberto, Bradley, Paul A., Baran, Andrzej S., Koester, Detlev, Bell, Keaton J., Romero, Alejandra D., Hermes, J. J., Fusillo, Nicola P. Gentile
The {\sl TESS} space mission has recently demonstrated its great potential to discover new pulsating white dwarf and pre-white dwarf stars, and to detect periodicities with high precision in already known white-dwarf pulsators. We report the discover
Externí odkaz:
http://arxiv.org/abs/2210.05486
Autor:
da Rosa, Gabriela Oliveira, Kepler, S. O., Córsico, Alejandro H., Costa, J. E. S., Hermes, J. J., Kawaler, S. D., Bell, Keaton J., Montgomery, M. H., Provencal, J. L., Winget, D. E., Handler, G., Dunlap, Bart, Clemens, J. C., Uzundag, Murat
PG 1159-035 is the prototype of the DOV hot pre-white dwarf pulsators. It was observed during the Kepler satellite K2 mission for 69 days in 59 s cadence mode and by the TESS satellite for 25 days in 20 s cadence mode. We present a detailed asterosei
Externí odkaz:
http://arxiv.org/abs/2208.04791
Autor:
Higgins, Michael E., Bell, Keaton J.
The Transiting Exoplanet Survey Satellite (TESS) has an exceptionally large plate scale of 21"/px, causing most TESS light curves to record the blended light of multiple stars. This creates a danger of misattributing variability observed by TESS to t
Externí odkaz:
http://arxiv.org/abs/2204.06020
Autor:
Vanderbosch, Zachary P., Hermes, J. J., Winget, Don E., Montgomery, Michael H., Bell, Keaton J., Nitta, Atsuko, Kepler, S. O.
We present a dedicated search for new pulsating helium-atmosphere (DBV) white dwarfs from the Sloan Digital Sky Survey using the McDonald 2.1m Otto Struve Telescope. In total we observed 55 DB and DBA white dwarfs with spectroscopic temperatures betw
Externí odkaz:
http://arxiv.org/abs/2201.09893