Hostname: page-component-7bb8b95d7b-pwrkn Total loading time: 0 Render date: 2024-09-13T04:30:02.018Z 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.

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