The expanding photosphere method: Progress and problems

József Vinkó; Katalin Takáts

doi:10.1063/1.2803597

The expanding photosphere method: Progress and problems

József Vinkó, Katalin Takáts

Exact Sciences School

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

5 Citations (Scopus)

Abstract

Distances to well-observed Type II-P SNe are determined from an updated version of the Expanding Photosphere Method (EPM), based on recent theoretical models. The new EPM distances show good agreement with other independent distances to the host galaxies without any significant systematic bias, contrary to earlier results in the literature. The accuracy of the method is comparable with that of the distance measurements for Type Ia SNe.

Original language	English
Title of host publication	SUPERNOVA 1987A
Subtitle of host publication	20 YEARS AFTER: Supernovae and Gamma-Ray Bursters
Pages	394-398
Number of pages	5
DOIs	https://doi.org/10.1063/1.2803597
Publication status	Published - 2007
Event	SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters - Aspen, CO, United States Duration: 19 Feb 2007 → 23 Feb 2007

Publication series

Name	AIP Conference Proceedings
Volume	937
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters
Country/Territory	United States
City	Aspen, CO
Period	19/02/07 → 23/02/07

Keywords

Core-collapse
Distances
Supernovae

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.2803597

Cite this

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title = "The expanding photosphere method: Progress and problems",

abstract = "Distances to well-observed Type II-P SNe are determined from an updated version of the Expanding Photosphere Method (EPM), based on recent theoretical models. The new EPM distances show good agreement with other independent distances to the host galaxies without any significant systematic bias, contrary to earlier results in the literature. The accuracy of the method is comparable with that of the distance measurements for Type Ia SNe.",

keywords = "Core-collapse, Distances, Supernovae",

author = "J{\'o}zsef Vink{\'o} and Katalin Tak{\'a}ts",

year = "2007",

doi = "10.1063/1.2803597",

language = "English",

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series = "AIP Conference Proceedings",

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T2 - SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters

AU - Vinkó, József

AU - Takáts, Katalin

PY - 2007

Y1 - 2007

N2 - Distances to well-observed Type II-P SNe are determined from an updated version of the Expanding Photosphere Method (EPM), based on recent theoretical models. The new EPM distances show good agreement with other independent distances to the host galaxies without any significant systematic bias, contrary to earlier results in the literature. The accuracy of the method is comparable with that of the distance measurements for Type Ia SNe.

AB - Distances to well-observed Type II-P SNe are determined from an updated version of the Expanding Photosphere Method (EPM), based on recent theoretical models. The new EPM distances show good agreement with other independent distances to the host galaxies without any significant systematic bias, contrary to earlier results in the literature. The accuracy of the method is comparable with that of the distance measurements for Type Ia SNe.

KW - Core-collapse

KW - Distances

KW - Supernovae

UR - http://www.scopus.com/inward/record.url?scp=36848999196&partnerID=8YFLogxK

U2 - 10.1063/1.2803597

DO - 10.1063/1.2803597

M3 - Conference contribution

AN - SCOPUS:36848999196

SN - 0735404488

SN - 9780735404489

T3 - AIP Conference Proceedings

SP - 394

EP - 398

BT - SUPERNOVA 1987A

Y2 - 19 February 2007 through 23 February 2007

ER -

The expanding photosphere method: Progress and problems

Abstract

Publication series

Other

Keywords

ASJC Scopus subject areas

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