Distance to the planetary nebula NGC 246 from the resolved companion of its central star

Howard E. Bond; Robin Ciardullo

doi:10.1086/316321

Distance to the planetary nebula NGC 246 from the resolved companion of its central star

Howard E. Bond, Robin Ciardullo

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

19 Scopus citations

Abstract

The central star of the planetary nebula NGC 246 is a resolved visual binary. We present CCD photometry of the G8 - K0 V companion, which is located 3″.8 from the hot nucleus. By fitting the companion to the zero-age main sequence, we derive a distance of d = 495⁺¹⁴⁵_-100 pc. This is one of the more secure distances known for a Galactic planetary nebula, but it could be improved still further with a better estimate of the metallicity of the system.

Original language	English (US)
Pages (from-to)	217-220
Number of pages	4
Journal	Publications of the Astronomical Society of the Pacific
Volume	111
Issue number	756
DOIs	https://doi.org/10.1086/316321
State	Published - Feb 1999

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/316321

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title = "Distance to the planetary nebula NGC 246 from the resolved companion of its central star",

abstract = "The central star of the planetary nebula NGC 246 is a resolved visual binary. We present CCD photometry of the G8 - K0 V companion, which is located 3″.8 from the hot nucleus. By fitting the companion to the zero-age main sequence, we derive a distance of d = 495+145-100 pc. This is one of the more secure distances known for a Galactic planetary nebula, but it could be improved still further with a better estimate of the metallicity of the system.",

author = "Bond, \{Howard E.\} and Robin Ciardullo",

year = "1999",

month = feb,

doi = "10.1086/316321",

language = "English (US)",

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pages = "217--220",

journal = "Publications of the Astronomical Society of the Pacific",

issn = "0004-6280",

publisher = "Institute of Physics Publishing",

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TY - JOUR

T1 - Distance to the planetary nebula NGC 246 from the resolved companion of its central star

AU - Bond, Howard E.

AU - Ciardullo, Robin

PY - 1999/2

Y1 - 1999/2

N2 - The central star of the planetary nebula NGC 246 is a resolved visual binary. We present CCD photometry of the G8 - K0 V companion, which is located 3″.8 from the hot nucleus. By fitting the companion to the zero-age main sequence, we derive a distance of d = 495+145-100 pc. This is one of the more secure distances known for a Galactic planetary nebula, but it could be improved still further with a better estimate of the metallicity of the system.

AB - The central star of the planetary nebula NGC 246 is a resolved visual binary. We present CCD photometry of the G8 - K0 V companion, which is located 3″.8 from the hot nucleus. By fitting the companion to the zero-age main sequence, we derive a distance of d = 495+145-100 pc. This is one of the more secure distances known for a Galactic planetary nebula, but it could be improved still further with a better estimate of the metallicity of the system.

UR - https://www.scopus.com/pages/publications/0033482592

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U2 - 10.1086/316321

DO - 10.1086/316321

M3 - Article

AN - SCOPUS:0033482592

SN - 0004-6280

VL - 111

SP - 217

EP - 220

JO - Publications of the Astronomical Society of the Pacific

JF - Publications of the Astronomical Society of the Pacific

IS - 756

ER -

Distance to the planetary nebula NGC 246 from the resolved companion of its central star

Abstract

All Science Journal Classification (ASJC) codes

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