arXiv Open Access 2022

Did a close tidal encounter cause the Great Dimming of Betelgeuse?

Hailey Aronson Thomas W. Baumgarte Stuart L. Shapiro
Lihat Sumber

Abstrak

We assess whether gravity darkening, induced by a tidal interaction during a stellar fly-by, might be sufficient to explain the Great Dimming of Betelgeuse. Adopting several simple approximations, we calculate the tidal deformation and associated gravity darkening in a close tidal encounter, as well as the reduction in the radiation flux as seen by a distant observer. We show that, in principle, the duration and degree of the resulting stellar dimming can be used to estimate the minimum pericenter separation and mass of a fly-by object, which, even if it remains undetected otherwise, might be a black hole, neutron star, or white dwarf. Our estimates show that, while such fly-by events may occur in other astrophysical scenarios, where our analysis should be applicable, they likely are not large enough to explain the Great Dimming of Betelgeuse by themselves.

Topik & Kata Kunci

Penulis (3)

H

Hailey Aronson

T

Thomas W. Baumgarte

S

Stuart L. Shapiro

Format Sitasi

Aronson, H., Baumgarte, T.W., Shapiro, S.L. (2022). Did a close tidal encounter cause the Great Dimming of Betelgeuse?. https://arxiv.org/abs/2201.08438

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2022
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓