About 433 results
AI Overview
Generating...
Sponsored
• AdSense Integration Active
💡
Did you mean:
star
Corrected by Entity Network
www.espncricinfo.com
espncricinfo.com › s...tars-2025-26-1522054
Women's Asia Cup Rising Stars 2026: Live scores, latest news, and exclusive player stats. See the full 2026 schedule and team standings here. Click for the latest updates!
arxiv.org
arxiv.org › abs › 2109.02246v2
From sector 1--44 {\em TESS} observations, 19 new roAp stars, 103 ostensibly non-peculiar stars with roAp-like frequencies and 617 $δ$~Scuti stars with independent frequencies typical of roAp stars w...
arxiv.org
arxiv.org › abs › 1903.06242v1
Our knowledge of the population of young (age
Sponsored
• AdSense Integration Active
arxiv.org
arxiv.org › abs › 1004.3121v2
We calculate NLTE models of stellar winds of hot compact stars (central stars of planetary nebulae and subdwarf stars). The studied range of subdwarf parameters is selected to cover a large part of th...
arxiv.org
arxiv.org › abs › astro-ph › 0210065v1
Using the method presented in Erspamer & North (2002, Paper I hereafter), detailed abundances of 140 stars are presented. The uncertainties characteristic of this method are presented and discussed. I...
arxiv.org
arxiv.org › abs › astro-ph › 0303018v1
We present new photometric data for seven high-amplitude delta Scuti stars. The observations were acquired between 1996 and 2002, mostly in the Johnson photometric system. For one star (GW UMa), our o...
arxiv.org
arxiv.org › abs › astro-ph › 0210516v1
We present a first set of results concerning stellar evolution of rotating low-mass stars. Our models include fully consistent transport of angular momentum and chemicals due to the combined action of...
arxiv.org
arxiv.org › abs › astro-ph › 0305141v1
We discuss the various post-main sequence phases of massive stars, focusing on Wolf-Rayet stars, Luminous Blue Variables, plus connections with other early-type and late-type supergiants. End states f...
arxiv.org
arxiv.org › abs › 2012.12152v1
The first multi-colour light curve models and period studies for the totally eclipsing W UMa stars TYC 3700-1384-1, V1511 Her and V1179 Her are presented. All three stars are A-subtype W UMa stars of ...
arxiv.org
arxiv.org › abs › astro-ph › 9809215v1
The mechanism for excitation of p-modes in rapidly oscillating, peculiar A (roAp, or cool chemically peculiar, CP) stars is unknown. Observations strongly suggest that acoustic modes in roAp stars are...
arxiv.org
arxiv.org › abs › astro-ph › 9602043v1
Witten's conjecture about strange quark matter (`Strange Matter') being the ground state of QCD at finite baryon number is presented and stars made of strange matter (`Strange Stars') are compared to ...
arxiv.org
arxiv.org › abs › astro-ph › 0609084v1
The winds of stars with very specific temperatures and luminosities are ideal for determining the magnitude and nature of mass loss in OB stars. I identify these stars and analyze their wind lines. Th...
www.reddit.com
reddit.com › r › Fauxm...and_oscar_nominated ›
...
arxiv.org
arxiv.org › abs › 1110.0548v1
We present a detailed abundance study of 11 RR Lyrae ab-type variables: AS Vir, BS Aps, CD Vel, DT Hya, RV Oct, TY Gru, UV Oct, V1645 Sgr, WY Ant, XZ Aps, and Z Mic.High resolution and high S/N echell...
en.wikipedia.org
en.wikipedia.org › wiki › Spying_Stars
Jayasundara's 'Turtle's Gaze on Spying Stars' Commences Shoot (EXCLUSIVE)". Variety. Retrieved 6 September 2025. "Spying Stars (Vimukthi Jayasundara)".
arxiv.org
arxiv.org › abs › astro-ph › 0111068v1
Massive OB stars play an important role in the evolution of molecular clouds and star forming regions. The OB stars both photo--ionize molecular gas as well as sweep up and compress interstellar gas t...
arxiv.org
arxiv.org › abs › 2203.02582v7
We study 119 B stars located in the Scorpius-Centaurus Association using data from NASA's TESS Mission. We see pulsations in 81 stars (68%) across the full range of effective temperatures. In particul...
arxiv.org
arxiv.org › abs › astro-ph › 9704220v1
We report detailed analysis of high-resolution spectra of nine high velocity metal-rich dwarfs in the solar neighborhood. The stars are super metal-rich and 5 of them have [Fe/H]>=+0.4, making them th...
arxiv.org
arxiv.org › abs › astro-ph › 0702251v1
I review recent results of the observations of magnetoacoustic p-mode oscillations in roAp stars with the focus on time-resolved spectroscopic studies. Time-series spectroscopy of roAp stars reveals u...
arxiv.org
arxiv.org › abs › 2312.04199v1
We present the results of a systematic search of the Transiting Exoplanet Survey Satellite (TESS) 2-min cadence data for new rapidly oscillating Ap (roAp) stars observed during the Cycle 2 phase of it...
