The relationship between HD 87892 and NGC 3132

Details The relationship between HD 87892 and NGC 3132 The relationship between HD 87892 and NGC 3132

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..411m&link_type=abstract

Astrophysical Journal, vol. 199, July 15, 1975, pt. 1, p. 411-417.

Astronomy and Astrophysics

Astrophysics

11

A Stars, Binary Stars, Planetary Nebulae, Stellar Spectrophotometry, Gas Ionization, Hot Stars, Interstellar Extinction, Radial Velocity, Tables (Data), Ubv Spectra

Scientific paper

The observations suggest that the central star of NGC 3132 is a double
system, the visually brighter component being HD 87892. The nebula is
ionized by a very hot object whose characteristics are briefly
discussed. The assumption that NGC 3132 lies at the same distance as HD
87892 leads to a very small ionized nebular mass.

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