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20012006
most citedThe Chemical Evolution of Helium in Globular Clusters: Implications for the Self-Pollution Scenario

69 citations · 169 across the 4 of their papers we have counts for

collaborators

17 papers

astro-ph200645 cited

An Evolutionary Model For Submillimeter Galaxies

Sukanya Chakrabarti, Yeshe Fenner, Lars Hernquist +2

[abridged]We calculate multi-wavelength spectral energy distributions (SEDs) (spanning optical to millimeter wavelengths) from simulations of major galaxy mergers with black hole f…

astro-ph200669 cited

The Chemical Evolution of Helium in Globular Clusters: Implications for the Self-Pollution Scenario

Amanda Karakas, Yeshe Fenner, Alison Sills +2

We investigate the suggestion that there are stellar populations in some globular clusters with enhanced helium (Y from 0.28 to 0.40) compared to the primordial value. We assume th…

astro-ph2006

Helium enhancements in globular cluster stars from Asymptotic Giant Branch star pollution

Amanda Karakas, Yeshe Fenner, Alison Sills +2

Using a chemical evolution model we investigate the intriguing suggestion that there are populations of stars in some globular clusters (e.g. NGC 2808, omega Centauri) with enhance…

astro-ph200655 cited

Cosmological implications of dwarf spheroidal chemical evolution

Yeshe Fenner, Brad K. Gibson, Roberto Gallino +1

The chemical properties of dwarf spheroidals in the local group are shown to be inconsistent with star formation being truncated after the reionization epoch (z~8). Enhanced levels…

astro-ph2005

Abundance Anomalies in NGC6752 - Do AGB Stars Have a Role?

S. W. Campbell, Y. Fenner, A. I. Karakas +2

We are in the process of testing a popular theory that the observed abundance anomalies in the Globular Cluster NGC 6752 are due to `internal pollution' from intermediate mass asym…

astro-ph2005

Galactic Chemical Evolution Redux: Atomic Numbers 6 < Z < 15

B. K. Gibson, Y. Fenner, A. Kiessling

Motivated by the inability of Galactic chemical evolution models to reproduce some of the observed solar neighbourhood distribution of elements (and isotopes) with atomic numbers 6…