Results 21 to 30 of about 261,811 (317)

A Well-Behaved Anisotropic Strange Star Model

open access: yesAdvances in Mathematical Physics, 2022
We obtain a new nonsingular exact model for compact stellar objects by using the Einstein field equations. The model is consistent with stellar star with anisotropic quark matter in the absence of electric field.
Amos V. Mathias, Jefta M. Sunzu
doaj   +1 more source

AGB Star Models [PDF]

open access: yesHighlights of Astronomy, 1992
AbstractAsymptotic giant branch star models are reviewed in relation to luminosity observations and chemical abundance observations of these stars.
openaire   +1 more source

ANALYTICAL MODELS FOR QUARK STARS [PDF]

open access: yesInternational Journal of Modern Physics D, 2007
We find two new classes of exact solutions to the Einstein–Maxwell system of equations. The matter content satisfies a linear equation of state consistent with quark matter; a particular form of one of the gravitational potentials is specified to generate solutions.
Komathiraj, K., Maharaj, S.D.
openaire   +3 more sources

Modelling Neutron-Star Ocean Dynamics

open access: yesUniverse, 2023
We revisit the calculation of mode oscillations in the ocean of a rotating neutron star, which may be excited during thermonuclear X-ray bursts. Our present theoretical understanding of ocean modes relies heavily on the traditional approximation commonly employed in geophysics. The approximation elegantly decouples the radial and angular sectors of the
Fabian Gittins   +3 more
openaire   +5 more sources

Star models with dark energy [PDF]

open access: yesGeneral Relativity and Gravitation, 2009
20 pages, 1 figure, references and some comments added, typos corrected, in press ...
Chan, R.   +2 more
openaire   +3 more sources

Modelling star cluster formation: Mergers

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
Abstract Star cluster formation in giant molecular clouds involves the local collapse of the cloud into small gas-rich subclusters, which can then subsequently collide and merge to build up the final star cluster(s). In this paper, we simulate collisions between these subclusters, using coupled smooth particle hydrodynamics for the gas ...
Jeremy Karam, Alison Sills
openaire   +2 more sources

Kajian Matriks Bobot Lokasi Model Space Time Autoregresi (STAR)

open access: yesJurnal Matematika Integratif, 2013
Model STAR (Space Time Autoregresi) merupakan pengembangan dari model deret waktu univariat AR (Autoregresi), menjadi model kombinasi lokasi dan waktu. Keterkaitan antar lokasi penelitian pada model STAR dinyatakan dengan matriks bobot W yang merupakan ...
Emah Suryamah   +2 more
doaj   +1 more source

RESEARCH ON MULTI-STAR NONLINEAR REGRESSION ESTIMATION MODEL OF SOIL MOISTURE BASED ON WAVELET ANALYSIS [PDF]

open access: yesThe International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, 2020
Soil moisture is an important parameter for studying meteorological, hydrological, and agricultural research. How to obtain accurate soil moisture has become a key issue.
Y. L. Pan   +7 more
doaj   +1 more source

Modeling Neutron Star Atmospheres

open access: yes, 2002
10 pages, 13 color figures; to be published in Proceedings of the 270. Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Bad Honnef (Germany), Jan. 21-25, 2002, eds. W. Becker, H.
Zavlin, V., Pavlov, G.
openaire   +3 more sources

Intermediate‐Mass Stars: Updated Models [PDF]

open access: yesThe Astrophysical Journal, 1999
A new set of stellar models in the mass range 1.2 to 9 $M_{\odot}$ is presented. The adopted chemical compositions cover the typical galactic values, namely $0.0001 \le Z \le 0.02$ and $0.23 \le Y \le 0.28$. A comparison among the most recent compilations of similar stellar models is also discussed.
Dominguez, Inma   +3 more
openaire   +2 more sources

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