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The Low Luminosity Central Star of the PN ESO166-21

Published online by Cambridge University Press:  07 August 2017

M.T. Ruiz ,
M. Peña  and
Torres-Peimbert
M.T. Ruiz
Affiliation:
Depto. de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile
M. Peña
Affiliation:
Instituto de Astronomia, Universidad Nacional Autónoma de México, Apdo. Postal 70 264, México D.F. 04510, México
Torres-Peimbert
Affiliation:
Instituto de Astronomia, Universidad Nacional Autónoma de México, Apdo. Postal 70 264, México D.F. 04510, México

Extract

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We present low dispersion UV and optical spectrophotometry of the central star of the PN ES0166–21. The stellar spectrum, from 1200 to 6600 Å, is a featureless continuum. The energy distribution is consistent with a black body of 120, 000 ± 20, 000K. The observed visual magnitude is 18.1.

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 500
Copyright
Copyright © Kluwer 1993 

References

Ruiz, M.T., Heathcote, S.R. and Weller, W.G. 1989, IAU symp. 131, 192 Google Scholar
Shaw, R.A. & Kaler, J.B. 1989, Ap. J. Supp. 69, 495 Google Scholar