Excess infrared radiation from the massive DAZ white dwarf GD 362: A debris disk?

Mukremin Kllic; Ted Von Hippel; S. K. Leggett; D. E. Winget

doi:10.1086/497825

Excess infrared radiation from the massive DAZ white dwarf GD 362: A debris disk?

Mukremin Kllic, Ted Von Hippel, S. K. Leggett, D. E. Winget

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

Original language	English
Pages (from-to)	L115-L118
Journal	Astrophysical Journal
Volume	632
Issue number	2 II
DOIs	https://doi.org/10.1086/497825
State	Published - Oct 20 2005
Externally published	Yes

ASJC Scopus Subject Areas

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Stars: individual (GD 362)
White dwarfs

Access to Document

10.1086/497825

Cite this

@article{5e28b1774f76414b9190f914176dae3a,

title = "Excess infrared radiation from the massive DAZ white dwarf GD 362: A debris disk?",

keywords = "Stars: individual (GD 362), White dwarfs",

author = "Mukremin Kllic and {Von Hippel}, Ted and Leggett, {S. K.} and Winget, {D. E.}",

year = "2005",

month = oct,

day = "20",

doi = "10.1086/497825",

language = "English",

volume = "632",

pages = "L115--L118",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "2 II",

}

TY - JOUR

T1 - Excess infrared radiation from the massive DAZ white dwarf GD 362

T2 - A debris disk?

AU - Kllic, Mukremin

AU - Von Hippel, Ted

AU - Leggett, S. K.

AU - Winget, D. E.

PY - 2005/10/20

Y1 - 2005/10/20

KW - Stars: individual (GD 362)

KW - White dwarfs

UR - http://www.scopus.com/inward/record.url?scp=30444461187&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=30444461187&partnerID=8YFLogxK

U2 - 10.1086/497825

DO - 10.1086/497825

M3 - Article

AN - SCOPUS:30444461187

SN - 0004-637X

VL - 632

SP - L115-L118

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 II

ER -

Excess infrared radiation from the massive DAZ white dwarf GD 362: A debris disk?

ASJC Scopus Subject Areas

Keywords

Access to Document

Other files and links

Cite this