Image de couverture de livre

A candidate period of 4.605 day for FRB 20121102A and one possible implication of its origin

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Li, Jixuan, Gao, Yang, Li, Di, Wu, Kinwah
Format:	Preprint
Publié:	2024
Sujets:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Alien Type Ia supernovae from the Milky Way merger history and one possible candidate: Kepler's supernova
par: He, Wenlang, et autres
Publié: (2025)

The VLBI spectrum of the persistent radio source associated with FRB 20190417A
par: Bruni, G., et autres
Publié: (2026)

Discovery of a PRS associated with FRB 20240114A
par: Bruni, G., et autres
Publié: (2024)

The Physical Properties of PS1-12sk and the implications for its Progenitor System
par: Mi, Kai-Li, et autres
Publié: (2026)

A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate
par: Luo, Changqing, et autres
Publié: (2024)

The orbital period changes for novae
par: Tang, Wenshi, et autres
Publié: (2025)

A gravitational wave detectable candidate Type Ia supernova progenitor
par: Chickles, Emma T., et autres
Publié: (2024)

A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
par: Li, Zhuowen, et autres
Publié: (2025)

The first extragalactic ultra-compact X-ray binary : a candidate black hole-white dwarf system
par: Ma, Qian-Qi, et autres
Publié: (2025)

Optical and Near-infrared Observations of SN 2023ixf for over 600 days after the Explosion
par: Li, Gaici, et autres
Publié: (2025)

Production of radioactive $^{22}$Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations
par: Pignatari, M., et autres
Publié: (2025)

Confirming Nunki as the closest core collapse progenitor candidate to the Sun
par: Waisberg, Idel, et autres
Publié: (2026)

A candidate to the long sought optical counterpart to the Rapid Burster in the bulge fossil fragment Liller 1
par: Pallanca, Cristina, et autres
Publié: (2025)

Localizing short-period pulsations in hard X-rays and Gamma-rays during an X9.0 flare
par: Li, Dong
Publié: (2025)

The fate of the failed supernova candidate M31-2014-DS1
par: Beasor, Emma R., et autres
Publié: (2026)

A comprehensive study of orbital evolution of LMC X-4: Existence of a second derivative of the orbital period
par: Jain, Chetana, et autres
Publié: (2024)

A disc wind origin for the optical spectra of dwarf novae in outburst
par: Tampo, Yusuke, et autres
Publié: (2024)

Probing solar modulation analytic models with cosmic ray periodic spectra
par: Long, Wei-Cheng, et autres
Publié: (2024)

SN 2023ixf: interaction signatures in the spectrum at 445 days
par: Folatelli, Gastón, et autres
Publié: (2025)

Timing analysis of a sample of five cataclysmic variable candidates observed by the XMM-Newton satellite
par: Nucita, A. A., et autres
Publié: (2026)

Tidal disruption event associated with the quasi-periodic eruptions from GSN 069: Possible disruption of a common envelope
par: Wang, Di
Publié: (2023)

A 2.9-hour periodic radio transient with an optical counterpart
par: Hurley-Walker, N., et autres
Publié: (2024)

Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
par: Sarkar, Arnab, et autres
Publié: (2024)

Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
par: Müller-Horn, Johanna, et autres
Publié: (2026)

Light curve modeling of the nearest neutron star candidate LAMOST J235456.73+335625.9
par: Han, Qing-bo, et autres
Publié: (2026)

On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7
par: Bamba, Aya, et autres
Publié: (2024)

The disc instability model: original recipe and additional ingredients
par: Hameury, Jean-Marie
Publié: (2025)

Violent mergers revisited: The origin of the fastest stars in the Galaxy
par: Pakmor, Rüdiger, et autres
Publié: (2025)

Quasi-periodic oscillations and reflection feature evolution in 4U 1630-47 observed with Insight-HXMT
par: Chen, Jiashi, et autres
Publié: (2025)

A binary model of long period radio transients and white dwarf pulsars
par: Horváth, Csanád, et autres
Publié: (2025)

Quasi-periodic oscillations of GHz-band polarization in a black hole
par: Wang, Wei, et autres
Publié: (2025)

Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova
par: Brennan, S. J., et autres
Publié: (2024)

A compact object with a K type star companion in the solar neighborhood: a wide post common envelope binary with a white dwarf candidate
par: Lin, Jie, et autres
Publié: (2026)

JWST reveals a luminous infrared source at the position of the failed supernova candidate N6946-BH1
par: Beasor, Emma R., et autres
Publié: (2023)

AstroSat and Insight-HXMT observations of the long-period X-ray pulsar 4U 2206+54
par: Epili, Prahlad R., et autres
Publié: (2024)

Gamma-ray lines, electron-positron annihilation, and possible radio emission in X-ray pulsars
par: Mushtukov, Alexander A., et autres
Publié: (2025)

SNR 1987A : Spitzer data from days 6000 to 8000 revisited
par: Bouchet, Patrice, et autres
Publié: (2025)

On the initial spin period distribution of neutron stars
par: Du, Shen-Shi, et autres
Publié: (2024)

AT 2018cow at ~5 years: additional evidence for a tidal disruption origin
par: Inkenhaag, Anne, et autres
Publié: (2025)

The origin of hypervelocity white dwarfs in the merger-disruption of He-CO white dwarfs
par: Glanz, Hila, et autres
Publié: (2024)