activity
20022005
collaborators

7 papers

astro-ph2005

The Stellar Halo Metallicity - Luminosity Relationship for Spiral Galaxies

Agostino Renda, Brad K. Gibson, Mustapha Mouhcine +4

The stellar halos of spiral galaxies bear important chemo-dynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations,…

astro-ph2004

On the origin of fluorine in the Milky Way

A. Renda, Y. Fenner, B. K. Gibson +6

The main astrophysical factories of fluorine (19F) are thought to be Type II supernovae, Wolf-Rayet stars, and the asymptotic giant branch (AGB) of intermediate mass stars. We pres…

astro-ph2004

Contrasting the chemical evolution of the Milky Way and Andromeda galaxies

Agostino Renda, Daisuke Kawata, Yeshe Fenner +1

The chemical evolution history of a galaxy hides clues about how it formed and has been changing through time. We have studied the chemical evolution history of the Milky Way (MW)…

astro-ph2004

Photometric Properties of White Dwarf Dominated Halos

H. -c. Lee, B. K. Gibson, Y. Fenner +5

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo…

astro-ph2003

Galactic Chemical Evolution

Brad K. Gibson, Yeshe Fenner, Agostino Renda +2

The primary present-day observables upon which theories of galaxy evolution are based are a system's morphology, dynamics, colour, and chemistry. Individually, each provides an imp…

astro-ph2003

Modelling the nova rate in galaxies

Francesca Matteucci, Agostino Renda, Antonio Pipino +1

We compute theoretical nova rates as well as type Ia SN rates in galaxies of different morphological type (Milky Way, ellipticals and irregulars) by means of detailed chemical evol…