Hostname: page-component-76fb5796d-dfsvx Total loading time: 0 Render date: 2024-04-25T20:49:57.578Z Has data issue: false hasContentIssue false
  • English
  • Français

Diffraction-limited speckle-masking observations of the Red Rectangle and IRC +10216 with the 6 m telescope

Published online by Cambridge University Press:  25 May 2016

R. Osterbart ,
Y. Y. Balega ,
G. Weigelt  and
N. Langer
R. Osterbart
Affiliation:
1Max-Planck–Institut für Radioastronomie, 53121 Bonn, Germany
Y. Y. Balega
Affiliation:
2Special Astrophysical Observatory, Zelenchukskaya Region, 357147 Russia
G. Weigelt
Affiliation:
1Max-Planck–Institut für Radioastronomie, 53121 Bonn, Germany
N. Langer
Affiliation:
3Max–Planck–Institut für Astrophysik, 85740 Garching, Germany

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.

We present the first diffraction-limited speckle-masking observations of the bipolar nebula Red Rectangle and of the carbon star IRC+10216. Both objects were observed with the SAO 6 m telescope in the NIR (resolution 0″.092) and the Red Rectangle with the ESO/MPG 2.2 m telescope in the red (resolution 0″.087).

Type
V. From AGB to Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 362
Copyright
Copyright © Kluwer 1997 

References

Fleischer, A.J., Gauger, A., Sedlmayr, E., 1995, A&A 297, 543.Google Scholar
Van Winckel, H., Waelkens, C., Waters, L.B.F.M., 1995, A&A 293, L25.Google Scholar
Yorke, H.W., Bodenheimer, P., Taam, R.E., 1995, ApJ 451, 308.CrossRefGoogle Scholar