Tracing Cosmic-Rays and SNe with Be Abundances

Details Tracing Cosmic-Rays and SNe with Be Abundances Tracing Cosmic-Rays and SNe with Be Abundances

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..195p&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 1, p. 195-198 (2002).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present the results of a new analysis of Be abundances in a large sample of stars, spanning the metallicity range -2.5 ≤ [Fe/H] ≤ - 0.7. The observations were taken with the Ultraviolet and Visible Echelle Spectrograph (UVES) at the ESO Very Large Telescope (VLT). With this new set of high quality data we aim at further investigating the trend of Be with metallicity, the possible presence of dispersion, and their implications for cosmic-ray and supernovae physics.

Affiliated with

Also associated with

No associations

Rating

Tracing Cosmic-Rays and SNe with Be Abundances 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 Tracing Cosmic-Rays and SNe with Be Abundances, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tracing Cosmic-Rays and SNe with Be Abundances will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-960480