Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...377..241n&link_type=abstract
Astronomy and Astrophysics, v.377, p.241-250 (2001)
Astronomy and Astrophysics
Astrophysics
3
Ism: Individual Objects: Ngc 3603, Planetary Nebulae: General, Planetary Nebulae: Individual: Pn G291.4-00.3
Scientific paper
In the vicinity of the southern hemisphere giant H II region NGC 3603 we discovered a new planetary nebula: PN G291.4-00.3 located at RAJ2000.0 = 11h14m32.1s +/- 0.3s, DECJ2000.0 = -61deg00'02'' +/- 1''. Monochromatic images reveal a central ring-like structure accompanied by onsets of arc-like filaments which might outline a bipolar outflow. Analysis of the nebula spectrum shows that helium and nitrogen are enriched, while oxygen, sulphur and argon abundances seem to be solar. The central star must be hot (above 100 kK) and having a luminosity of more than 3000 Lsun. All evidence shows that PN G291.4-00.3 is a high-excitation, density bounded planetary nebula of the type I, coming from the high-mass end of the intermediate mass stars. Based on observations obtained at the European Southern Observatory, La Silla, Chile.
Durand Stephane
Els Sebastian
Köppen Joachim
Nürnberger Dieter
Stanke Th.
No associations
LandOfFree
PN G291.4-00.3: A new type I planetary nebula 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 PN G291.4-00.3: A new type I planetary nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and PN G291.4-00.3: A new type I planetary nebula will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1099745