Image de couverture de livre

The Red Supergiant Progenitor of the Type II Supernova 2024abfl

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Luo, Jingxiao, Zhang, Lifu, Chen, Bing-Qiu, Cheng, Qiyuan, Guo, Boyang, Li, Jiao, Guo, Yanjun, Xiong, Jianping, Meng, Xiangcun, Chen, Xuefei, Liu, Zhengwei, Han, Zhanwen
Format:	Preprint
Publié:	2024
Sujets:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

SN2024abfl: A Low-Luminosity Type IIP Supernova at the Low-Mass End of Core Collapse
par: Li, Luhan, et autres
Publié: (2026)

The Red Supergiant Progenitor of Type II Supernova 2024ggi
par: Xiang, Danfeng, et autres
Publié: (2024)

Red Supergiants as Supernova Progenitors
par: Van Dyk, Schuyler D.
Publié: (2025)

Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
par: Guo, Boyang, et autres
Publié: (2025)

Mass, Luminosity, and Stellar Age of Early-type Stars from the LAMOST Survey
par: Li, Qida, et autres
Publié: (2025)

Pre-Supernova Eruptions Triggered by Sudden Energy Deposition in Low-Mass Core-Collapse Supernova Progenitors
par: Zha, Shuai, et autres
Publié: (2026)

Surface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)
par: Xiong, Jianping, et autres
Publié: (2025)

Type Ia Supernovae from First-generation Stars
par: Li, Zhenwei, et autres
Publié: (2024)

The Binary Fraction of B-type Runaway Stars from LAMOST DR8
par: Chen, Kun, et autres
Publié: (2025)

Identifying Hierarchically Triple Star Systems with Gaia DR3 and LAMOST
par: He, Tongyu, et autres
Publié: (2024)

Identification of false positive double-lined spectroscopic binaries in LAMOST-MRS data due to moonlight contamination
par: Wang, Zhoulin, et autres
Publié: (2026)

Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
par: Luo, Jingxiao, et autres
Publié: (2024)

Adiabatic Mass Loss In Binary Stars. IV. Low and Intermediate Mass Helium Binary Stars
par: Zhang, Lifu, et autres
Publié: (2024)

The First Photometric Analysis of Two Low Mass Ratio Contact Binary Systems In TESS Survey
par: Cheng, Qiyuan, et autres
Publié: (2024)

Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer -- Application in High Mass X-ray Binaries
par: Ge, Hongwei, et autres
Publié: (2024)

Formation of extremely low-mass white dwarf binaries undergoing enhanced angular momentum loss
par: Zhao, Ziqi, et autres
Publié: (2026)

SN 2024abfl: A Low-Luminosity Type IIP Supernova in NGC 2146 from a Low-Mass Red Supergiant Progenitor
par: Chen, Xiaohan, et autres
Publié: (2026)

A New Pathway to Single Be Stars: Ejected Companions from Type Ia Supernovae
par: Bao, Yuchen, et autres
Publié: (2026)

The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star
par: Kilpatrick, Charles D., et autres
Publié: (2025)

Multi-wavelength Signatures of Supernova Shock Breakout from Red Supergiants in Two Dimensions
par: Chen, Wun-Yi, et autres
Publié: (2025)

Discoveries and Properties of EL CVn-type Binaries in the TESS Survey
par: Xiong, Jianping, et autres
Publié: (2024)

The Progenitor of the Type II-Plateau SN 2025pht in NGC 1637: The Dustiest, Most Luminous Red Supergiant So Far?
par: Van Dyk, Schuyler D., et autres
Publié: (2026)

Molecules and Chemistry in Red Supergiants
par: Ziurys, Lucy M., et autres
Publié: (2025)

TV Mon -- post mass transfer Algol type binary with $δ$ Scuti pulsations in primary component
par: Kovalev, Mikhail, et autres
Publié: (2024)

Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-Resolution Survey
par: Guo, Sufen, et autres
Publié: (2025)

Type Ia Supernova Progenitors and Surviving Companions within the Symbiotic Channel
par: Wang, Yu-Hui, et autres
Publié: (2025)

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST
par: Li, Jiangdan, et autres
Publié: (2026)

The Formation of Electron-capture Supernovae: A Review
par: Wang, Bo, et autres
Publié: (2025)

The new compact triple system: discovery of bright third star around contact binary using LAMOST-MRS spectra and photometry
par: Kovalev, Mikhail, et autres
Publié: (2025)

Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova
par: Healy, Sarah, et autres
Publié: (2023)

Type Ia Supernova Progenitor Properties and Their Host Galaxies
par: Chakraborty, Sudeshna, et autres
Publié: (2023)

SN 2024iss: Double-Peaked Light Curves and Implications for a Yellow Supergiant Progenitor
par: Yamanaka, Masayuki, et autres
Publié: (2025)

Direct Detection of Type II-P Supernova Progenitors with the Euclid and CSST Surveys
par: Wu, Junjie, et autres
Publié: (2026)

SN 2022acko and the Properties of its Red Supergiant Progenitor: Direct Detection, Light Curves, and Nebular Spectroscopy
par: Teixeira, Gabriel, et autres
Publié: (2025)

The Binary Fraction of Red Supergiants in the Magellanic Clouds
par: Dai, Min, et autres
Publié: (2025)

Red Supergiants in the Milky Way and Nearby Galaxies
par: Bonanos, Alceste Z.
Publié: (2025)

Modeling the Progenitor Stars of Observed IIP Supernovae
par: You, Kai-An, et autres
Publié: (2024)

The Red Supergiant Problem: As Seen from the Local Group's Red Supergiant Populations
par: Healy, Sarah, et autres
Publié: (2024)

Weak-CN Stars Are Ordinary Cool Red Supergiants
par: Ting, Yuan-Sen, et autres
Publié: (2026)

Searching for Galactic Red Supergiants with Gaia RVS Spectra
par: Zhang, Zehao, et autres
Publié: (2024)