The changing spectrum of the LMC planetary N66

Details The changing spectrum of the LMC planetary N66 The changing spectrum of the LMC planetary N66

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..876c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 106, no. 702, p. 876-878

Astronomy and Astrophysics

Astronomy

1

Astronomical Photometry, Magellanic Clouds, Planetary Nebulae, Star Formation, Brightness Distribution, Hubble Space Telescope, Rosat Mission, Wolf-Rayet Stars, X Ray Astronomy, X Ray Sources

Scientific paper

Recent spectroscopy and photometry of the planetary nebula N66 (SMP 83) in the Large Magellanic Cloud show a continuing evolution, with a central WR spectrum becoming more visible. The planetary nebula shell and Wolf-Rayet (WR) star have velocities which differ by approximately 240 km/s. Properties of this interesting object are reviewed, and we discuss its possible X-ray detection by ROSAT.

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