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Unusual Emission Line Profiles of M1-1

Published online by Cambridge University Press:  19 July 2016

Katsunori Shibata
Affiliation:
Astronomical Institute, Tohoku University, Aobayama, SENDAI 980, Japan
Shin'ichi Tamura
Affiliation:
Astronomical Institute, Tohoku University, Aobayama, SENDAI 980, Japan

Extract

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In order to seek out intrinsically compact PN, we have observed high-excitation and angularly small PN, M1-1, with the intensified Reticon system (one-dimensional 1024 pixel-array) at the Coude focus of the 188 cm telescope. We have obtained highly resolved emission line profiles of [NII]λ6583, Hα, [OIII]λ5007, and HeIIλ4686 at several slit position angles. These lines were analyzed with the aid of Multiple Gaussian Method. From the analysis of their radial velocities and decomposed profiles, we can summarize our observational results as follows, (a) HeII were fitted by three Gaussians, those are main blue and red-components and an extremely red-shifted sub-component. Hα and [OIII] were decomposed into blue and red components. [NII] were fitted by single Gaussian.

Type
II. Nebular Properties
Copyright
Copyright © Kluwer 1989