Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other objects

Details Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other objects Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other objects

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26...90m&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Scientific paper

We have estimated the magnitude and time variation of the radial
abundance gradients using planetary nebulae, open clusters, cepheids and
other young objects. We concluded that the gradients have flattened out
in the last 8 Gyr, with important consequences for models of the
chemical evolution of the Galaxy.

Affiliated with

Also associated with

No associations

Rating

Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other 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 Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial abundance gradients as observational constraints of galactic evolution: planetary nebulae and other objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1478723