A new model for V838 Monocerotis: A born-again object including an episode of accretion

T. M. Lawlor

doi:10.1111/j.1365-2966.2005.09230.x

A new model for V838 Monocerotis: A born-again object including an episode of accretion

T. M. Lawlor

Penn State Brandywine

Research output: Contribution to journal › Review article › peer-review

24 Scopus citations

Abstract

We present new stellar evolution models that show that the born-again phenomenon, also known as a very late thermal pulse, is a viable explanation for the behaviour of V838 Monocerotis if a period of accretion is included. Based on this model, we assert that V838 Mon is a variation of a born-again giant in close orbit with a main-sequence binary companion of mass greater than 0.7 M⊙.

Original language	English (US)
Pages (from-to)	695-700
Number of pages	6
Journal	Monthly Notices of the Royal Astronomical Society
Volume	361
Issue number	2
DOIs	https://doi.org/10.1111/j.1365-2966.2005.09230.x
State	Published - Aug 1 2005

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1111/j.1365-2966.2005.09230.x

Cite this

@article{dd4612eb952b4bcd8fe23af0d2caf02b,

title = "A new model for V838 Monocerotis: A born-again object including an episode of accretion",

abstract = "We present new stellar evolution models that show that the born-again phenomenon, also known as a very late thermal pulse, is a viable explanation for the behaviour of V838 Monocerotis if a period of accretion is included. Based on this model, we assert that V838 Mon is a variation of a born-again giant in close orbit with a main-sequence binary companion of mass greater than 0.7 M⊙.",

author = "Lawlor, \{T. M.\}",

year = "2005",

month = aug,

day = "1",

doi = "10.1111/j.1365-2966.2005.09230.x",

language = "English (US)",

volume = "361",

pages = "695--700",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

TY - JOUR

T1 - A new model for V838 Monocerotis

T2 - A born-again object including an episode of accretion

AU - Lawlor, T. M.

PY - 2005/8/1

Y1 - 2005/8/1

N2 - We present new stellar evolution models that show that the born-again phenomenon, also known as a very late thermal pulse, is a viable explanation for the behaviour of V838 Monocerotis if a period of accretion is included. Based on this model, we assert that V838 Mon is a variation of a born-again giant in close orbit with a main-sequence binary companion of mass greater than 0.7 M⊙.

AB - We present new stellar evolution models that show that the born-again phenomenon, also known as a very late thermal pulse, is a viable explanation for the behaviour of V838 Monocerotis if a period of accretion is included. Based on this model, we assert that V838 Mon is a variation of a born-again giant in close orbit with a main-sequence binary companion of mass greater than 0.7 M⊙.

UR - https://www.scopus.com/pages/publications/23444447128

UR - https://www.scopus.com/pages/publications/23444447128#tab=citedBy

U2 - 10.1111/j.1365-2966.2005.09230.x

DO - 10.1111/j.1365-2966.2005.09230.x

M3 - Review article

AN - SCOPUS:23444447128

SN - 0035-8711

VL - 361

SP - 695

EP - 700

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

A new model for V838 Monocerotis: A born-again object including an episode of accretion

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this