Results 31 to 40 of about 562,063 (305)

XMM-Newton X-ray study of early type stars in the Carina OB1 association [PDF]

open access: yes, 2007
<p><b>Aims:</b> X-ray properties of the stellar population in the Carina OB1 association are examined with special emphasis on early-type stars.
I. I. Antokhin   +14 more
core   +1 more source

A Magnetospheric Dichotomy for Pulsars with Extreme Inclinations

open access: yesUniverse, 2021
In this work, we expand on a comment by Lyne et al. (2017), that intermittent pulsars tend to congregate near a stripe in the logarithmic period versus period-derivative diagram.
Fan Zhang
doaj   +1 more source

Looking at the Stars

open access: yesTheoretical Computer Science, 2004
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Elena Prieto-Rodriguez, Christian Sloper
openaire   +6 more sources

The Evolutionary Statuses of Solar Type Detached Eclipsing Binary Stars [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2012
We presented fundamental stellar parameters and evolutionary statuses of six solar type detached eclipsing binaries whose masses are in the range of 0.97-1.43 M⊙. EK Cep and FL Lyr belong to the zero age main sequence.
Chanisa Kanjanascul   +5 more
doaj   +1 more source

Implications for compact stars of a soft nuclear equation of state from heavy-ion data [PDF]

open access: yes, 2012
We study the implications on compact star properties of a soft nuclear equation of state determined from kaon production at subthreshold energies in heavy-ion collisions.
Sagert, Irina   +10 more
core   +1 more source

From synthetic SEDs to stellar origins: A deep learning model for physical parameter retrieval in hot subdwarf stars

open access: yesAstronomy & Astrophysics
Aims. The formation mechanisms of spectrally diverse hot subdwarfs remain unclear. While existing mass distribution analyses suggest additional channels beyond helium white dwarf (He-WD) mergers contribute to He-rich subdwarf formation, these conclusions
Feng Mengqi   +6 more
doaj   +1 more source

The State Complexity of Star-Complement-Star [PDF]

open access: yes, 2012
We resolve an open question by determining matching (asymptotic) upper and lower bounds on the state complexity of the operation that sends a language L to (c(L*))*, where c() denotes complement.
Galina Jirásková, Jeffrey O. Shallit
openaire   +2 more sources

How to Create a STARS Account for Students [PDF]

open access: yes, 2020
Instructions detailing how to create an account for STARS for studentshttps://stars.library.ucf.edu/stars-documentation/1014/thumbnail ...
Bottorff, Kerri
core  

Radial-velocity measurements of subdwarf B stars [PDF]

open access: yes, 2011
Subdwarf B (sdB) stars are hot, subluminous stars which are thought to be core-helium burning with thin hydrogen envelopes. The mechanism by which these stars lose their envelopes has been controversial, but it has been argued that binary star ...
Copperwheat, CM   +14 more
core   +1 more source

Rainbow’s stars [PDF]

open access: yesThe European Physical Journal C, 2017
In recent years, a growing interest on the equilibrium of compact astrophysical objects like white dwarf and neutron stars has been manifested. In particular, various modifications due to Planck scale energy effects have been considered. In this paper we analyze the modification induced by Gravity's Rainbow on the equilibrium configurations described ...
Garattini, Remo, Mandanici, Gianluca
openaire   +3 more sources

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