Zobrazeno 1 - 4
of 4
pro vyhledávání: '"M. J. Walentosky"'
Autor:
Alexander Staron, M. J. Walentosky, Benjamin Blankartz, Stephen Alexander, Tristan Clark, Justin Messinger
Publikováno v:
The Astrophysical Journal. 835:233
We present a new computational method for calculating the motion of stars in a dwarf spheroidal galaxy (dSph) that can use either Newtonian gravity or Modified Newtonian Dynamics (MOND). In our model, we explicitly calculate the motion of several tho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47a96ae41a1054c7f150695d9f2a5500
https://doi.org/10.3847/1538-4357/835/2/233
https://doi.org/10.3847/1538-4357/835/2/233
Autor:
Richard A. Wade, Drew R. Clausen, Ravi Kumar Kopparapu, Richard O’Shaughnessy, M. A. Stark, M. J. Walentosky, Vicky Kologera, Marc van der Sluys
Publikováno v:
AIP Conference Proceedings.
Observations to date preferentially find Galactic hot subdwarf (sdB/sdO) stars in binaries when the subdwarfs are more luminous than their relatively faint companions (G/K/M dwarfs, white dwarfs). As suggested by Han et al. [1], this selection bias m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8287dd5ed2433ffeedc6112da86ef81f
https://doi.org/10.1063/1.3536419
https://doi.org/10.1063/1.3536419
Autor:
Steve B. Howell, D. W. Hoard, C. Brinkworth, S. Kafka, M. J. Walentosky, Frederick M. Walter, T. A. Rector
Using Spitzer Space Telescope photometric observations of the eclipsing, interacting binary WZ Sge, we have discovered that the accretion disk is far more complex than previously believed. Our 4.5 and 8 micron time series observations reveal that the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ccf93c1fd09df24aaa5767242b06661
https://resolver.caltech.edu/CaltechAUTHORS:HOWapj08
https://resolver.caltech.edu/CaltechAUTHORS:HOWapj08
Autor:
S. G. Alexander, M. J. Walentosky, Justin Messinger, Alexander Staron, Benjamin Blankartz, Tristan Clark
Publikováno v:
Astrophysical Journal; 2/1/2017, Vol. 835 Issue 2, p1-1, 1p