Zobrazeno 1 - 10
of 947
pro vyhledávání: '"M. Shara"'
Autor:
Michael M. Shara, Kenneth M. Lanzetta, Alexandra Masegian, James T. Garland, Stefan Gromoll, Joanna Mikolajewska, Mikita Misiura, David Valls-Gabaud, Frederick M. Walter, John K. Webb
Publikováno v:
The Astrophysical Journal Letters, Vol 977, Iss 2, p L48 (2024)
A century or less separates the thermonuclear-powered eruptions of recurrent novae (RNe) in the hydrogen-rich envelopes of massive white dwarfs. The colliding ejecta of successive RN events are predicted to always generate very large (tens of parsecs
Externí odkaz:
https://doaj.org/article/70bfc2b1931c49a2b317e9fd3c5de6d0
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 518:5279-5297
Accurate determination of the rates of nova eruptions in different kinds of galaxies gives us strong constraints on those galaxies’ underlying white dwarf and binary populations, and those stars’ spatial distributions. Until 2016, limitations inh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::405e27c6a122731744fe4f9441dae4f2
https://doi.org/10.1093/mnras/stac2960
https://doi.org/10.1093/mnras/stac2960
Akademický článek
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Publikováno v:
Geoscientific Model Development, Vol 17, Pp 8093-8114 (2024)
The accurate parameterization of atmospheric surface layer processes is crucial for weather forecasts using numerical weather prediction models. Here, an attempt has been made to improve the surface layer parameterization in the Weather Research and
Externí odkaz:
https://doaj.org/article/ed23ce16f57a49819f1c1232bc22695a
Autor:
Erez Michaely, Michael M. Shara
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 502:4540-4546
Multiple star systems interact strongly with Galactic field stars when the outer semi-major axis of a triple or multiple star is > 10 3 AU. Stable triples composed of two white-dwarfs (WD) and a low mass main sequence (MS) star in a wide outer orbit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32a2e5b862645cbdc9dca92076f3fd97
https://doi.org/10.1093/mnras/stab339
https://doi.org/10.1093/mnras/stab339
Autor:
Catherine M. Broome, Jon P. Fryzek, Lauren C. Bylsma, Meghan E. Mitchell, Nawar M. Shara, Stephen J. Fernandez, Joseph P. Catlett, Todd L. Edwards, Daniel J. Hausrath, Loren P. Lipworth, Jacob S. Lai, Kathy Dong, Naval Daver, Carl E. Allen
Publikováno v:
Blood. 140:5490-5491
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::af622ece56251d09f166d9323a41b60f
https://doi.org/10.1182/blood-2022-167819
https://doi.org/10.1182/blood-2022-167819
Publikováno v:
Advances in Space Research. 66:1072-1079
Direct determination of WD masses in CVs is extremely difficult, which is the reason very few direct determinations exist. We present a method for calculating an estimate of WD masses in CVs and of the rate at which they accrete matter from their com
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::47f8a87e84ab29a919bb4497eddea995
https://doi.org/10.1016/j.asr.2019.08.029
https://doi.org/10.1016/j.asr.2019.08.029
Autor:
Nawar M. Shara, Sameer Desale, Barbara V. Howard, Zeid Diab, Wm. James Howard, Lyle G. Best, Wenyu Wang, Elisa T. Lee, Richard B. Devereux, Xiyao Ai, Jason G. Umans
Publikováno v:
Journal of Nephrological Science. 2:5-14
American Indians (AI) have a high prevalence of diabetes, obesity, cardiovascular disease (CVD), and chronic kidney disease. Inclusion of kidney function and other population-specific characteristics in equations used to predict atherosclerotic CVD (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c865344d1980b71181dca3131d38b8e
https://doi.org/10.29245/2767-5149/2020/1.1103
https://doi.org/10.29245/2767-5149/2020/1.1103
Publikováno v:
Nature Astronomy. 4:886-892
The envelopes accreted by white dwarf stars from their hydrogen-rich companions1 experience thermonuclear-powered runaways2,3 observed as classical nova eruptions4,5 peaking at 105–106 solar luminosities6–9. Virtually all nova progenitors—‘no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3ab64350bbd29209f505ca2bf370790d
https://doi.org/10.1038/s41550-020-1062-y
https://doi.org/10.1038/s41550-020-1062-y
Autor:
Kenneth M. Lanzetta, Stefan Gromoll, Michael M. Shara, Stephen Berg, David Valls-Gabaud, Frederick M. Walter, John K. Webb
Publikováno v:
Publications of the Astronomical Society of the Pacific. 135:015002
The “Condor Array Telescope” or “Condor” is a high-performance “array telescope” comprised of six apochromatic refracting telescopes of objective diameter 180 mm, each equipped with a large-format, very low-read-noise (≈1.2 e−), very
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c0e50a81a490b348dc54db5d67ab6d37
https://doi.org/10.1088/1538-3873/acaee6
https://doi.org/10.1088/1538-3873/acaee6