Moozonian

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 Cricket Scores, Schedule & News
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
Rapidly-oscillating {\it TESS} A--F main sequence stars: are the roAp stars a distinct class?
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
The Early Evolution of Stars and Exoplanet Systems: Exploring and Exploiting Nearby, Young Stars (an Astro2020 Science White Paper)
Our knowledge of the population of young (age
Sponsored • AdSense Integration Active
arxiv.org
arxiv.org › abs › 1004.3121v2
NLTE wind models of hot subdwarf stars
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
Automated spectroscopic abundances of A and F-type stars using echelle spectrographs II. Abundances of 140 A-F stars from ELODIE and CORALIE
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
A photometric monitoring of bright high-amplitude delta Scuti stars. II. Period updates for seven stars
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
Rotational mixing in low-mass stars : I Effect of the mu-gradients in main sequence and subgiant Pop I stars
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
Massive Stars in Transition
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
Photometric analysis of three totally eclipsing W UMa stars with increasing periods: TYC 3700-1384-1, V1511 Her and V1179 Her
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
A magnetic model for acoustic modes in roAp stars
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
Strange stars: Which is the ground stage of QCD at finite baryon number
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
Looking for Mister Goodstar (A preliminary analysis of stars with S IV, V and VI wind lines)
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...
arxiv.org
arxiv.org › abs › 1110.0548v1
The Chemical Compositions of Variable Field Horizontal Branch Stars: RR Lyrae Stars
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
Spying Stars - Wikipedia
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
The Impact of Massive Stars on the Formation of Young Stellar Clusters
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
Pulsating B stars in the Scorpius-Centaurus Association with TESS
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
High-Resolution Abundance Analysis of Very Metal-Rich Stars in the Solar Neighborhood
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
Observations of pulsations in roAp stars
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
TESS Cycle 2 observations of roAp stars with 2-min cadence data
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...