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Planetary nebula spectra in M 60 and M 82

Published online by Cambridge University Press:  30 August 2012

Roberto H. Méndez ,
Ana M. Teodorescu ,
Takashi Hattori ,
Laura Magrini  and
Lent C. Johnson
Roberto H. Méndez
Affiliation:
1Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA email: [email protected], [email protected]
Ana M. Teodorescu
Affiliation:
1Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA email: [email protected], [email protected]
Takashi Hattori
Affiliation:
Subaru Telescope, Nat. Astr. Obs. of Japan, Hilo, Hawaii, USA
Laura Magrini
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Firenze, Italy
Lent C. Johnson
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, USA
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Abstract

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Using the Subaru telescope and its FOCAS spectrograph in multi-object mode, we have obtained spectra of a selection of bright PNs in two galaxies: the Virgo giant elliptical M 60 (NGC 4649), and the starburst spiral M 82. We report on individual extinctions, as determined from the Balmer decrement, and also on the intensities of [O III] 4959 and 5007 relative to Hβ.

Keywords

galaxies: individual (NGC 4649, M 82)dustextinctionplanetary nebulae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 434 - 435
Copyright
Copyright © International Astronomical Union 2012

References

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