The Nature of M 2-29

Details The Nature of M 2-29 The Nature of M 2-29

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391..107g&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

Astronomy and Astrophysics

Astronomy

Scientific paper

The hydrogen deficient central star of the PN M2-29 exhibited an R
CrB-like brightness minimum, but much longer-lasting. The nebula
consists of a nearly spherical ring and a monopolar jet-like structure.
The images and spectra collected by us show a surprisingly static nebula
surrounding a WELS star in a binary system.

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