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High Dispersion Spectroscopy of the PN K 648 in the Globular Cluster M 15

Published online by Cambridge University Press:  15 December 2006

Akito Tajitsu  and
Masaaki Otsuka
Akito Tajitsu
Affiliation:
Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720, USA email: tajitsu@subaru.naoj.org
Masaaki Otsuka
Affiliation:
Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, 3037-5 Kamogata Honjo, Asaguchi, Okayama 719-0232, Japan
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Abstract

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We present our recent results of the high dispersion spectroscopy of a Galactic halo planetary nebula, K 648, in the globular cluster M 15. The position-velocity diagrams of our spectra indicate the existence of collimated outflows in K 648. In the [N II$\lambda$6583 diagram, we found high velocity components with a velocity $\sim$60 km s$^{-1}$ in the central region of K648.

Keywords

planetary nebulae: individual (K 648 = Ps 1)globular clusters: individual (M 15)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 523 - 524
Copyright
© 2006 International Astronomical Union