Results 71 to 80 of about 170,850 (201)
Constraints on the Formation of M31’s Stellar Halo from the SPLASH Survey
The SPLASH (Spectroscopic and Photometric Landscape of Andromeda’s Stellar Halo) Survey has observed fields throughout M31’s stellar halo, dwarf satellites, and stellar disk.
Karoline Gilbert
doaj +1 more source
Solar and stellar rotation [PDF]
Workshop on Solar and Stellar Physics through Eclipses -- MAR 27-29, 2006 -- Ankara Univ, ORSEM Campus, Side, Antalya, TURKEYThe secular evolution of the stellar rotation through angular momentum loss, driven by the stellar wind, and the consequences of ...
Demircan, O., Filiz-Ak, N., Eker, Z.
core +1 more source
Chaotic Dynamics of Stellar Spin in Binaries and the Production of Misaligned Hot Jupiters
Motivated by observed hot Jupiter systems with high stellar obliquities, we examine the dynamics of stellar spin in planetary systems with distant stellar companions, with inclinations sufficiently high so that the planet undergoes Kozai-Lidov ...
Anderson Kassandra R. +2 more
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Exploring central star variability of planetary nebulae using gaia photometry
This study presents an analysis of the variability of 81 central stars of planetary nebulae (CSPNe) are identified as variable in Gaia Data Release 3 (DR3).
M. A. NegmEldin +3 more
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This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
openaire +2 more sources
The µ Herculis system solved after nearly three centuries
Context. µ Herculis is a bright, nearby quadruple system. Its brightest member, µ Her Aa, displays solar-like oscillations, establishing the system as a crucial benchmark for asteroseismology, provided that its mass can be determined independently of ...
Marcussen Marcus L. +13 more
doaj +1 more source
Benchmarking pre-main sequence stellar evolutionary tracks using disk-based dynamical stellar masses
Stellar masses are a fundamental property to understand models of pre-main sequence evolution, but their values derived from Hertzsprung–Russell (HR) diagrams are strongly model dependent.
Zallio Luigi +16 more
doaj +1 more source
Reverse Shock Revisited in Cassiopeia A with Chandra
Using data from the Chandra X-ray Observatory, we revisit the reverse shock in the supernova remnant (SNR) Cassiopeia A. Based on spectroscopy of a series of annuli in the northwest (NW) and southeast (SE), we get the radial profiles of the S/Si K α line
Yin Wu, X. J. Yang
doaj +1 more source
Discovery of the first octupole pulsation mode in a δ Scuti star
Aims. We attempt to understand better how stellar pulsations in close binary systems are affected, and possibly induced, by tidal, Coriolis, and centrifugal forces. Methods.
Rappaport S. A. +10 more
doaj +1 more source
STEllAR-GROUP/hpx: HPX V1.2.0: The C++ Standards Library for Parallelism and Concurrency
<p>Please see here for all changes: <a href="https://stellar-group.github.io/hpx/docs/sphinx/tags/1.2.0/html/releases/whats_new_1_2_0.html">https://stellar-group.github.io/hpx/docs/sphinx/tags/1.2.0/html/releases/whats_new_1_2_0.html</a>
Shoshana Jakobovits +30 more
core +1 more source

