Constraints on the progenitor of cassiopeia A

Patrick A. Young; Chris L. Fryer; Aimee Hungerford; David Arnett; Gabriel Rockefeller; F. X. Timmes; Benedict Voit; Casey Meakin; Kristoffer A. Eriksen

doi:10.1086/500108

Constraints on the progenitor of cassiopeia A

Patrick A. Young, Chris L. Fryer, Aimee Hungerford, David Arnett, Gabriel Rockefeller, F. X. Timmes, Benedict Voit, Casey Meakin, Kristoffer A. Eriksen

Steward Observatory

Research output: Contribution to journal › Article › peer-review

142 Scopus citations

Abstract

We compare a suite of three-dimensional explosion calculations and stellar models incorporating advanced physics with observational constraints on the progenitor of Cassiopeia A. We consider binary and single stars from 16 to 40 M_⊙ with a range of explosion energies and geometries. The parameter space allowed by observations of nitrogen-rich high-velocity ejecta, ejecta mass, compact remnant mass, and ⁴⁴Ti and ⁵⁶Ni abundances individually and as an ensemble is considered. A progenitor of 15-25 M_⊙ that loses its hydrogen envelope to a binary interaction and undergoes an energetic explosion can match all the observational constraints.

Original language	English (US)
Pages (from-to)	891-900
Number of pages	10
Journal	Astrophysical Journal
Volume	640
Issue number	2 I
DOIs	https://doi.org/10.1086/500108
State	Published - Apr 1 2006

Keywords

Hydrodynamics
Nuclear reactions, nucleosynthesis, abundances
Stars: Evolution
Supernova remnants
Supernovae: individual (Cassiopeia A)

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1086/500108

Cite this

@article{095cf838bba84faba04a843899f28aa4,

title = "Constraints on the progenitor of cassiopeia A",

abstract = "We compare a suite of three-dimensional explosion calculations and stellar models incorporating advanced physics with observational constraints on the progenitor of Cassiopeia A. We consider binary and single stars from 16 to 40 M⊙ with a range of explosion energies and geometries. The parameter space allowed by observations of nitrogen-rich high-velocity ejecta, ejecta mass, compact remnant mass, and 44Ti and 56Ni abundances individually and as an ensemble is considered. A progenitor of 15-25 M⊙ that loses its hydrogen envelope to a binary interaction and undergoes an energetic explosion can match all the observational constraints.",

keywords = "Hydrodynamics, Nuclear reactions, nucleosynthesis, abundances, Stars: Evolution, Supernova remnants, Supernovae: individual (Cassiopeia A)",

author = "Young, {Patrick A.} and Fryer, {Chris L.} and Aimee Hungerford and David Arnett and Gabriel Rockefeller and Timmes, {F. X.} and Benedict Voit and Casey Meakin and Eriksen, {Kristoffer A.}",

year = "2006",

month = apr,

day = "1",

doi = "10.1086/500108",

language = "English (US)",

volume = "640",

pages = "891--900",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "2 I",

}

TY - JOUR

T1 - Constraints on the progenitor of cassiopeia A

AU - Young, Patrick A.

AU - Fryer, Chris L.

AU - Hungerford, Aimee

AU - Arnett, David

AU - Rockefeller, Gabriel

AU - Timmes, F. X.

AU - Voit, Benedict

AU - Meakin, Casey

AU - Eriksen, Kristoffer A.

PY - 2006/4/1

Y1 - 2006/4/1

N2 - We compare a suite of three-dimensional explosion calculations and stellar models incorporating advanced physics with observational constraints on the progenitor of Cassiopeia A. We consider binary and single stars from 16 to 40 M⊙ with a range of explosion energies and geometries. The parameter space allowed by observations of nitrogen-rich high-velocity ejecta, ejecta mass, compact remnant mass, and 44Ti and 56Ni abundances individually and as an ensemble is considered. A progenitor of 15-25 M⊙ that loses its hydrogen envelope to a binary interaction and undergoes an energetic explosion can match all the observational constraints.

AB - We compare a suite of three-dimensional explosion calculations and stellar models incorporating advanced physics with observational constraints on the progenitor of Cassiopeia A. We consider binary and single stars from 16 to 40 M⊙ with a range of explosion energies and geometries. The parameter space allowed by observations of nitrogen-rich high-velocity ejecta, ejecta mass, compact remnant mass, and 44Ti and 56Ni abundances individually and as an ensemble is considered. A progenitor of 15-25 M⊙ that loses its hydrogen envelope to a binary interaction and undergoes an energetic explosion can match all the observational constraints.

KW - Hydrodynamics

KW - Nuclear reactions, nucleosynthesis, abundances

KW - Stars: Evolution

KW - Supernova remnants

KW - Supernovae: individual (Cassiopeia A)

UR - http://www.scopus.com/inward/record.url?scp=33645837024&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33645837024&partnerID=8YFLogxK

U2 - 10.1086/500108

DO - 10.1086/500108

M3 - Article

AN - SCOPUS:33645837024

SN - 0004-637X

VL - 640

SP - 891

EP - 900

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 I

ER -

Constraints on the progenitor of cassiopeia A

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this