activity
19972007
most citedConnecting the primordial and Galactic deuterium abundances

46 citations · 46 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph200746 cited

Connecting the primordial and Galactic deuterium abundances

Gary Steigman, Donatella Romano, Monica Tosi

The deuterium abundances inferred from observations of the interstellar medium within 1-2 kpc of the Sun range over a factor of three and the corresponding oxygen abundances show a…

astro-ph2004

Quantifying the uncertainties of chemical evolution studies. I. The stellar initial mass function and the stellar lifetimes

Donatella Romano, Cristina Chiappini, Francesca Matteucci +1

The stellar initial mass function and the stellar lifetimes are basic ingredients of chemical evolution models, for which different recipes can be found in the literature. In this…

astro-ph2000

Chemical and dynamical evolution in gas-rich dwarf galaxies

Simone Recchi, Francesca Matteucci, Annibale D'Ercole

We study the effect of a single, instantaneous starburst in a gas-rich dwarf galaxy on the dynamical and chemical evolution of its interstellar medium. We consider the energetic in…

astro-ph1998

Evidence for inverse Compton emission in the powerful radio galaxy 3C 219

G. Brunetti, A. Comastri, G. Setti +1

Spectral analysis of ROSAT PSPC and ASCA archive data and a recent ROSAT HRI observation of the powerful FRII radio galaxy 3C 219 reveal an absorbed point-like source, coincident w…

astro-ph1998

BeppoSax Spectral Survey of soft X-ray selected BL Lacs

A. Wolter, A. Comastri, G. Ghisellini +10

We present X-ray spectra obtained with BeppoSAX (Satellite per Astronomia X) of 10 BL Lac objects, selected from the Einstein Medium Sensitivity and Slew Surveys. We find that in a…

astro-ph1997

ASCA detection of the FeK edge in the spectrum of the Seyfert 2 galaxy IRAS 04575-7537: a sign of a complex absorber

C. Vignali, A. Comastri, G. M. Stirpe +5

ASCA X-ray spectral analysis of the Seyfert 2 galaxy IRAS 04575-7537 is presented. The main result is the presence of a significant iron edge at a rest energy of 7.13^+0.21_-0.16 k…