Zobrazeno 1 - 10
of 2 873
pro vyhledávání: '"Interior Models"'
Autor:
Albalahi, Abeer M.1 (AUTHOR), Yousaf, Z.2 (AUTHOR) zeeshan.math@pu.edu.pk, Khan, S.2 (AUTHOR), Ali, Akbar1 (AUTHOR)
Publikováno v:
European Physical Journal C -- Particles & Fields. Sep2024, Vol. 84 Issue 9, p1-11. 11p.
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 84, Iss 9, Pp 1-11 (2024)
Abstract This work explores the construction of spherically symmetric models of stellar interiors by incorporating the null complexity factor (CF) as an additional constraint. This supplementary condition helps us to close an array of stellar structu
Externí odkaz:
https://doaj.org/article/628956e96c874009b3e83a5769112357
Autor:
Bailey, Elizabeth, Stevenson, David J.
Interior models of Uranus and Neptune often assume discrete layers, but sharp interfaces are expected only if major constituents are immiscible. Diffuse interfaces could arise if accretion favored a central concentration of the least volatile constit
Externí odkaz:
http://arxiv.org/abs/2012.04166
Autor:
Péters, Marie-Julie, Maistre, Sébastien Le, Yseboodt, Marie, Marty, Jean-Charles, Rivoldini, Attilio, Van Hoolst, Tim, Dehant, Véronique
Two years after InSight's arrival at Mars, the ExoMars 2020 mission will land on the opposite side of the red planet. Similarly to InSight, which carries the RISE (Rotation and Interior Structure Experiment) radio-science experiment, the ExoMars miss
Externí odkaz:
http://arxiv.org/abs/1910.10588
Autor:
Péters, M.-J., Le Maistre, S., Yseboodt, M., Marty, J.-C., Rivoldini, A., Van Hoolst, T., Dehant, V.
Publikováno v:
In Planetary and Space Science January 2020 180
An exoplanet's structure and composition are first-order controls of the planet's habitability. We explore which aspects of bulk terrestrial planet composition and interior structure affect the chief observables of an exoplanet: its mass and radius.
Externí odkaz:
http://arxiv.org/abs/1510.07582
Autor:
ÇELİK ORHAN, Zeynep
Publikováno v:
Volume: 22, Issue: 2 262-267
Afyon Kocatepe Üniversitesi Fen Ve Mühendislik Bilimleri Dergisi
Afyon Kocatepe Üniversitesi Fen Ve Mühendislik Bilimleri Dergisi
The stellar interior models are generally used to understand the structure and evolution of stars. The models that best represent the stars are decided by the observation parameters. For this purpose, the output data of the models obtained are compar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0f8a7859314ce2c6c99bdb35fdaa2ba
https://doi.org/10.35414/akufemubid.1068872
https://doi.org/10.35414/akufemubid.1068872
Autor:
ÇELİK ORHAN, Zeynep
Publikováno v:
Afyon Kocatepe University Journal of Science & Engineering / Afyon Kocatepe Üniversitesi Fen Ve Mühendislik Bilimleri Dergisi; nis2022, Vol. 22 Issue 2, p262-267, 6p
Autor:
Zhang, Q. S.
The convective overshoot mixing plays an important role in stellar structure and evolution. However, the overshoot mixing is a long standing problem. The uncertainty of the overshoot mixing is one of the most uncertain factors in stellar physics. As
Externí odkaz:
http://arxiv.org/abs/1303.0139