Hostname: page-component-54dcc4c588-rz4zl Total loading time: 0 Render date: 2025-10-02T12:40:41.231Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectrophotometry and Kinematics of the Newly Discovered PN in the Outher Field of the LMC

Published online by Cambridge University Press:  07 August 2017

M.A. Dopita ,
E. Vassiliadis  and
D.H. Morgan
M.A. Dopita
Affiliation:
Mt. Stromlo and Siding Springs Observatories, Institute of Advanced Studies, The Australian National University, Canberra
E. Vassiliadis
Affiliation:
Mt. Stromlo and Siding Springs Observatories, Institute of Advanced Studies, The Australian National University, Canberra
D.H. Morgan
Affiliation:
The Royal Observatory, Blackford Hill, Edinburgh

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recently a number of new planetary nebulae (PN) have been found in the outer field of the LMC using deep objective–prism J plates taken with a Schmidt Telescope at the AAO. For a number of these PN, we have obtained spectrophotometry on the 2.3m ATT and for a sub–sample, determined the radial velocities using the Echelle Spectrograph of the 2.3m Telescope. All this data is to appear in the ApJ.

Information

Type
VI. Planetary Nebulae in Galactic Systems
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 569
Copyright
Copyright © Kluwer 1993