Zobrazeno 1 - 10
of 67
pro vyhledávání: '"Bill Paxton"'
Autor:
Nishan Tchekmedyian, MD, Bill Paxton, MD, PhD, Francois Lebel, MD, Lena Keossayan, BA, John V. Heymach, MD, PhD
Publikováno v:
JTO Clinical and Research Reports, Vol 1, Iss 4, Pp 100081- (2020)
Externí odkaz:
https://doaj.org/article/c8d34ceb341d421196b3ea04c4014128
Non-invasive prenatal chromosomal aneuploidy testing--clinical experience: 100,000 clinical samples.
Autor:
Ron M McCullough, Eyad A Almasri, Xiaojun Guan, Jennifer A Geis, Susan C Hicks, Amin R Mazloom, Cosmin Deciu, Paul Oeth, Allan T Bombard, Bill Paxton, Nilesh Dharajiya, Juan-Sebastian Saldivar
Publikováno v:
PLoS ONE, Vol 9, Iss 10, p e109173 (2014)
OBJECTIVE: As the first laboratory to offer massively parallel sequencing-based noninvasive prenatal testing (NIPT) for fetal aneuploidies, Sequenom Laboratories has been able to collect the largest clinical population experience data to date, includ
Externí odkaz:
https://doaj.org/article/111113173d1246f08e586fb0b3a90399
Publikováno v:
JTO Clinical and Research Reports
JTO Clinical and Research Reports, Vol 1, Iss 4, Pp 100081-(2020)
JTO Clinical and Research Reports, Vol 1, Iss 4, Pp 100081-(2020)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2695221fb24a08d2360c31283dd0c852
http://europepmc.org/articles/PMC8474396
http://europepmc.org/articles/PMC8474396
Massive stars undergo fundamental-mode and first-overtone radial pulsations with periods of 100-1000 days as Red Supergiants (RSGs). At large amplitudes, these pulsations substantially modify the outer envelope's density structure encountered by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7f0c4cdead30e895bc1a6f92ea9770d
http://arxiv.org/abs/2001.07303
http://arxiv.org/abs/2001.07303
Autor:
Lars Bildsten, William M. Wolf, A. Gautschy, Richard H. D. Townsend, Robert Farmer, Matteo Cantiello, Anne Thoul, Shashi M. Kanbur, Jared A. Goldberg, Michael Zhang, Aaron Dotter, Josiah Schwab, Pablo Marchant, Francis Timmes, Radosław Smolec, Adam S. Jermyn, Bill Paxton
Publikováno v:
The Astrophysical Journal. Supplement Series, 243(1):10. IOP Publishing Ltd.
We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA). RSP is a new functionality in MESAstar that models the non-linear radial stellar pulsations that characterize RR Lyrae, Cephe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::418256d52823005c534bfb0ab89523f4
https://dare.uva.nl/personal/pure/en/publications/modules-for-experiments-in-stellar-astrophysics-mesa(3ecc9e94-88fd-466c-9af2-9941f5bf1de5).html
https://dare.uva.nl/personal/pure/en/publications/modules-for-experiments-in-stellar-astrophysics-mesa(3ecc9e94-88fd-466c-9af2-9941f5bf1de5).html
We present advances in modeling Type IIP supernovae using MESA for evolution to shock breakout coupled with STELLA for generating light and radial velocity curves. Explosion models and synthetic light curves can be used to translate observable proper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86afc146d0921224e66d182995de1107
http://arxiv.org/abs/1903.09114
http://arxiv.org/abs/1903.09114
Autor:
Josiah Schwab, Jared Brooks, Lars Bildsten, Elena Sorokina, Bill Paxton, Eliot Quataert, Sergei Blinnikov
We study the evolution and final outcome of long-lived (${\approx}10^5$ years) remnants from the merger of a He white dwarf (WD) with a more massive C/O or O/Ne WD. Using Modules for Experiments in Stellar Astrophysics ($\texttt{MESA}$), we show that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfbaf809ba513cbe33b74a9e66368d14
http://arxiv.org/abs/1710.09464
http://arxiv.org/abs/1710.09464
Accretion-induced collapse (AIC) occurs when an O/Ne white dwarf (WD) grows to nearly the Chandrasekhar mass ($M_{\rm Ch}$), reaching central densities that trigger electron captures in the core. Using Modules for Experiments in Stellar Astrophysics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b89ecb6bccd81252e84d1e1f5d13a44
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 440:1274-1280
Figure 1: The highest masses of the CO cores and the lowest masses of the ONe cores (top), and the initial masses of the stars that produce the highest CO core masses and the lowest ONe core masses (bottom), all plotted against the carbon burning rat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::85c9c0b524dafca79f578fa4a624ba70
https://doi.org/10.1093/mnras/stu108
https://doi.org/10.1093/mnras/stu108
Autor:
Saul Rappaport, Lorne Nelson, Ph. Podsiadlowski, Bill Paxton, Eric Pfahl, Nikku Madhusudhan, Stephen Justham
We have computed models for ultraluminous X-ray sources ("ULXs") consisting of a black-hole accretor of intermediate mass ("IMBH"; e.g., ~1000 Msun) and a captured donor star. For each of four different sets of initial donor masses and orbital separa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f6074c8d4c50a963b569985201db1d4
https://doi.org/10.1086/500238
https://doi.org/10.1086/500238