Zobrazeno 1 - 10
of 2 494
pro vyhledávání: '"Montgomery M."'
Autor:
Kao, Malia L., Hawkins, Keith, Rogers, Laura K., Bonsor, Amy, Dunlap, Bart H., Sanders, Jason L., Montgomery, M. H., Winget, D. E.
White dwarfs (WDs) polluted by exoplanetary material provide the unprecedented opportunity to directly observe the interiors of exoplanets. However, spectroscopic surveys are often limited by brightness constraints, and WDs tend to be very faint, mak
Externí odkaz:
http://arxiv.org/abs/2405.17667
Autor:
Montgomery, M. H., Dunlap, Bart H.
Accurate models of cooling white dwarfs must treat the energy released as their cores crystallize. This phase transition slows the cooling by releasing latent heat and also gravitational energy, which results from phase separation: liquid C is releas
Externí odkaz:
http://arxiv.org/abs/2312.11647
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
Publikováno v:
EPJ Web of Conferences, Vol 152, p 01012 (2017)
White dwarfs represent the end point of stellar evolution for the majority of stars. As such, they are excellent astrophysical laboratories. They are structurally simple, with electron degenerate cores surrounded by thin surface layers of helium and/
Externí odkaz:
https://doaj.org/article/fb6771c1a1e74d778c27fa5a40420ac9
Autor:
Wood M. A., Simpson J. C., Kawaler S. D., O'Brien M. S., Nather R. E., Metcalfe T. S., Winget D. E., Montgomery M., Jiang X. J., Leibowitz E. M., Ibbetson P., O'Donoghue D., Krzesinski J., Pajdosz G., Zola S., Vauclair G., Dolez N., Chevreton M.
Publikováno v:
Open Astronomy, Vol 9, Iss 2, Pp 211-222 (2000)
Externí odkaz:
https://doaj.org/article/a9e4e1fd563d4a5283c546427f00f124
Publikováno v:
Open Astronomy, Vol 9, Iss 1, Pp 97-112 (2000)
Externí odkaz:
https://doaj.org/article/283954f7d15340eebb8ec2abbdd82fd1
Autor:
Montgomery M. H., Winget D. E.
Publikováno v:
Open Astronomy, Vol 9, Iss 1, Pp 23-32 (2000)
Externí odkaz:
https://doaj.org/article/5df24b0bf9fa4863a2ba74f3c84afcda
Publikováno v:
Open Astronomy, Vol 9, Iss 1, Pp 87-96 (2000)
Externí odkaz:
https://doaj.org/article/79df15d467b84beab650dc405b7ed5b9
Publikováno v:
Open Astronomy, Vol 7, Iss 2, Pp 183-196 (1998)
Externí odkaz:
https://doaj.org/article/590721ca61924ba0b0c5caefcd7d5fb3