Search for envelopes of some stellar planetary nebulae, symbiotic stars and further emission-line objects

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Planetary Nebulae: General, Stars: Symbiotic, Stars: Novae, Stars: Horizontal Branch

Scientific paper

At 17 emission-line objects, mainly PN, the seeing disc has been compared with that of some surrounding stars (CCD frames taken through B, V, R, [OIII] 5007 Angstroms and H alpha filters). Nebulosities were found at: CPD-53.8315 degrees (0.5" in x-direction, 0.4" in y-direction), H^2-2 (0.3", 1.4") and CPD-56.8032 degrees (1.3", 1.3"). Further small nebulosities are possible at MWC 560, MWC 574, LS IV-12.111 degrees and HR Del, but they should be considered as rather uncertain. Besides, the known outer nebula at CPD-53.8315 degrees (2 condensations, 11.6" separation, PA = 146 degrees) was observed, and the author discovered a circular halo of 50" around Hb 6 - both outer nebulosities visible in the light of H alpha. Based on observations collected at the European Southern Observatory at La Silla, Chile.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Search for envelopes of some stellar planetary nebulae, symbiotic stars and further emission-line objects does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Search for envelopes of some stellar planetary nebulae, symbiotic stars and further emission-line objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for envelopes of some stellar planetary nebulae, symbiotic stars and further emission-line objects will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1683145

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.