X-ray observations of planetary nebulae with binary nuclei

K. M.V. Apparao; G. D. Berthiaume; J. A. Nousek

doi:10.1086/171809

X-ray observations of planetary nebulae with binary nuclei

K. M.V. Apparao
, G. D. Berthiaume
, J. A. Nousek

Astronomy & Astrophysics

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

10 Scopus citations

Abstract

Einstein and EXOSAT satellite observations of X-ray emission from the planetary nebulae A63 and LoTr 5 are reviewed. Both of these systems contain binary central stars. No flux was detected from A63 (central star UU Sge). LoTr 5 (central star IN Com) is a previously unreported X-ray emitter; it showed no statistically significant X-ray variability. Three models for the source of the X-ray emission in such systems are considered in the light of these and previous results.

Original language	English (US)
Pages (from-to)	534-536
Number of pages	3
Journal	Astrophysical Journal
Volume	397
Issue number	2
DOIs	https://doi.org/10.1086/171809
State	Published - 1992

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/171809

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title = "X-ray observations of planetary nebulae with binary nuclei",

abstract = "Einstein and EXOSAT satellite observations of X-ray emission from the planetary nebulae A63 and LoTr 5 are reviewed. Both of these systems contain binary central stars. No flux was detected from A63 (central star UU Sge). LoTr 5 (central star IN Com) is a previously unreported X-ray emitter; it showed no statistically significant X-ray variability. Three models for the source of the X-ray emission in such systems are considered in the light of these and previous results.",

author = "Apparao, \{K. M.V.\} and Berthiaume, \{G. D.\} and Nousek, \{J. A.\}",

year = "1992",

doi = "10.1086/171809",

language = "English (US)",

volume = "397",

pages = "534--536",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

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TY - JOUR

T1 - X-ray observations of planetary nebulae with binary nuclei

AU - Apparao, K. M.V.

AU - Berthiaume, G. D.

AU - Nousek, J. A.

PY - 1992

Y1 - 1992

N2 - Einstein and EXOSAT satellite observations of X-ray emission from the planetary nebulae A63 and LoTr 5 are reviewed. Both of these systems contain binary central stars. No flux was detected from A63 (central star UU Sge). LoTr 5 (central star IN Com) is a previously unreported X-ray emitter; it showed no statistically significant X-ray variability. Three models for the source of the X-ray emission in such systems are considered in the light of these and previous results.

AB - Einstein and EXOSAT satellite observations of X-ray emission from the planetary nebulae A63 and LoTr 5 are reviewed. Both of these systems contain binary central stars. No flux was detected from A63 (central star UU Sge). LoTr 5 (central star IN Com) is a previously unreported X-ray emitter; it showed no statistically significant X-ray variability. Three models for the source of the X-ray emission in such systems are considered in the light of these and previous results.

UR - https://www.scopus.com/pages/publications/11944263294

UR - https://www.scopus.com/pages/publications/11944263294#tab=citedBy

U2 - 10.1086/171809

DO - 10.1086/171809

M3 - Article

AN - SCOPUS:11944263294

SN - 0004-637X

VL - 397

SP - 534

EP - 536

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

X-ray observations of planetary nebulae with binary nuclei

Abstract

All Science Journal Classification (ASJC) codes

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