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27 April 2024
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992
for query "
M. Marconi
". (0.00 sec.)
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1.
Improvement of the CORS method for Cepheids radii determination based on Stromgren photometry
A. Ruoppo
;
V. Ripepi
;
M. Marconi
;
G. Russo
;
20 Apr 2004
/ Astron.Astrophys. 422 (2004) 253-265
2.
Classical Cepheid Pulsation Models. X. The Period-Age Relation
G. Bono
;
M. Marconi
;
S. Cassisi
;
F. Caputo
;
W. Gieren
;
G. Pietrzynski
;
29 Nov 2004
/ Astrophys.J. 621 (2005) 966-977
3.
RR Lyrae stars in Galactic globular clusters.III. Pulsational predictions for metal content Z=0.0001 to Z=0.006
Di Criscienzo
;
M.
;
M. Marconi
;
F. Caputo
;
21 May 2004
/ Astrophys.J. 612 (2004) 1092-1106
4.
Bright metal-poor variables: why "Anomalous" Cepheids?
F. Caputo
;
V. Castellani
;
S. Degl'Innocenti
;
G. Fiorentino
;
M. Marconi
;
20 May 2004
5.
A pulsational approach to near infrared and visual magnitudes of RR Lyrae stars
G. Bono
;
F. Caputo
;
V. Castellani
;
M. Marconi
;
J. Storm
;
S. Degl'Innocenti
;
6 Jun 2003
/ Mon.Not.Roy.Astron.Soc. 344 (2003) 1097
6.
Theoretical models for classical Cepheids. VIII. Effects of helium and heavy elements abundance on the Cepheid distance scale
G. Fiorentino
;
F. Caputo
;
M. Marconi
;
I. Musella
;
10 May 2002
/ Astrophys.J. 576 (2002) 402-412
7.
On the pulsation parallax of the variable star RR Lyr
G. Bono
;
F. Caputo
;
V. Castellani
;
M. Marconi
;
J. Storm
;
15 Apr 2002
/ Mon.Not.Roy.Astron.Soc. 332 (2002) L78
8.
Theoretical models for Bump Cepheids
G. Bono
;
V. Castellani
;
M. Marconi
;
8 Dec 2001
9.
The Cepheid Period-Luminosity relation and the maser distance to NGC 4258
F. Caputo
;
M. Marconi
;
I. Musella
;
24 Oct 2001
10.
Improving the mass determination of Galactic Cepheids
G. Bono
;
W.P. Gieren
;
M. Marconi
;
P. Fouque'
;
F. Caputo
;
16 Aug 2001
11.
Theoretical insights into the RR Lyrae K-band Period-Luminosity relation
G. Bono
;
F. Caputo
;
V. Castellani
;
M. Marconi
;
28 May 2001
/ Mon.Not.Roy.Astron.Soc. 326 (2001) 1183
12.
On the second overtone stability among SMC Cepheids
G. Bono
;
F. Caputo
;
M. Marconi
;
7 Mar 2001
/ Mon.Not.Roy.Astron.Soc. 325 (2001) 1353
13.
Classical Cepheid Pulsation Models. III. The Predictable Scenario
G. Bono
;
V. Castellani
;
M. Marconi
;
2 Aug 1999
14.
RR Lyrae variables in M5 as a test of pulsational theory
F. Caputo
;
V. Castellani
;
M. Marconi
;
V. Ripepi
;
19 Feb 1999
15.
Theoretical stellar models for old galactic clusters
V. Castellani
;
S. Degl'Innocenti
;
M. Marconi
;
5 Dec 1998
16.
On the Period-Luminosity-Color Relation of Classical Cepheids
G. Bono
;
M. Marconi
;
28 Oct 1998
17.
Theoretical Models for Classical Cepheids: II. Period-Luminosity, Period-Color and Period-Luminosity-Color Relations
G. Bono
;
F. Caputo
;
V. Castellani
;
M. Marconi
;
10 Sep 1998
18.
On the distance of Magellanic Clouds: first overtone Cepheids
G. Bono
;
M.A.T. Groenewegen
;
M. Marconi
;
F. Caputo
;
6 Jun 2002
19.
Recent results on Pre-main sequence delta Scuti stars
V. Ripepi
;
M. Marconi
;
F. Palla
;
S. Bernabei
;
A. Ruoppo
;
F. Cusano
;
J.M. Alcala'
;
3 Oct 2005
20.
Intermediate-mass star models with different helium and metal contents
G. Bono
;
F. Caputo
;
S. Cassisi
;
M. Marconi
;
L. Piersanti
;
A. Tornambe'
;
19 Jun 2000
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