Welcome to my home page (still under construction). I am associate astronomer at the astronomical observatory of Rome. I am also affiliated to the Istituto di Astrofisica Spaziale e Fisica Cosmica CNR (IASF) . My (research and personal) interests are:
| Stellar structure and evolution | astrophysics of light elements | Interacting binaries evolution | |
| Formation of stars and pre-MS evolution | lithium in brown dwarfs and AGB | Globular Clusters | |
| Family | |||
|---|---|---|---|

Here you will find

2002: my html presentation at the
Stellar Abundances & Nucleosynthesis Conference (Seattle, 27-29 March
2002) is here
1999-2000: Research Activity
in Italian,
and in English,
plus an update 2001
and list of publication
a list
of
my publications as found in the ADS
my recent papers with links, to get preprints
Mazzitelli, D'Antona and Caloi 1995, AA, 302, 382
Silvestri, F., Ventura, P., D'Antona, F. and Mazzitelli, I. 1998,
ApJ 509, 192
Montalban,J., D'Antona, F. and Mazzitelli, I. 2000, A&A
A project of research on ``Astrophysics of light elements" coordinated by F.
D'Antona has been financed for 1997-98 from the CNAA (Consorzio Nazionale
Astronomia ed Astrofisica). A small meeting gathering the participants in
this project has been held in Monte Porzio on 16 - 17 April 1998.
The program of this workshop
How to contact me:
by mail at
dantona_AT_mporzio.astro.it
by snail mail: write to Francesca D'Antona, Osservatorio Astronomico di
Roma,
via dell' Osservatorio 2, 00040 Monteporzio (RM) Italy.
by telephone +39-6-94286447 or fax: +39-6-9447243
Per Giampaolo Josefina e Paolo
PREMAIN
SEQUENCE 1994 tracks by D'Antona and Mazzitelli
PREMAIN
SEQUENCE 1997 tracks by D'Antona and Mazzitelli
PREMAIN
SEQUENCE 1998 UPDATE tracks by D'Antona and Mazzitelli
GLOBULAR CLUSTERS TURNOFF ISOCHRONES AND HORIZONTAL BRANCH MODELS
from
Caloi, D'Antona and Mazzitelli 1997, AA, 320, 823
D'Antona, Caloi and and Mazzitelli 1997, ApJ, 477, 519
GLOBULAR CLUSTERS LUMINOSITY FUNCTIONS
from
GLOBULAR CLUSTERS ISOCHRONES DOWN TO VERY LOW MASS STARS
from
TURNOFF ISOCHRONES FOR POPULATION I MODELS FROM 0.6 TO 15 MSUN
from
ASTROFISICA DEGLI ELEMENTI LEGGERI
is given here.
M15 in observed bands
M92 in observed bands
M15 and M92 with chosen distances and zero reddening in observed bands