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20 February 2020
 
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Results 1 to 20 of 810 for query "M. Marconi". (0.02 sec.)

[    1    2    3    4    5    10    ]   Next
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
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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
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3.
Bright metal-poor variables: why "Anomalous" Cepheids?
F. Caputo; V. Castellani; S. Degl'Innocenti; G. Fiorentino; M. Marconi;
20 May 2004
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4.
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
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5.
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
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6.
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
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7.
Theoretical models for Bump Cepheids
G. Bono; V. Castellani; M. Marconi;
8 Dec 2001
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8.
The Cepheid Period-Luminosity relation and the maser distance to NGC 4258
F. Caputo; M. Marconi; I. Musella;
24 Oct 2001
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9.
Improving the mass determination of Galactic Cepheids
G. Bono; W.P. Gieren; M. Marconi; P. Fouque'; F. Caputo;
16 Aug 2001
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10.
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
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11.
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
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12.
Classical Cepheid Pulsation Models. III. The Predictable Scenario
G. Bono; V. Castellani; M. Marconi;
2 Aug 1999
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13.
RR Lyrae variables in M5 as a test of pulsational theory
F. Caputo; V. Castellani; M. Marconi; V. Ripepi;
19 Feb 1999
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14.
Theoretical stellar models for old galactic clusters
V. Castellani; S. Degl'Innocenti; M. Marconi;
5 Dec 1998
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15.
On the Period-Luminosity-Color Relation of Classical Cepheids
G. Bono; M. Marconi;
28 Oct 1998
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16.
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
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17.
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
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18.
On the distance of Magellanic Clouds: first overtone Cepheids
G. Bono; M.A.T. Groenewegen; M. Marconi; F. Caputo;
6 Jun 2002
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19.
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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20.
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
- - -
21.
Multisite observations of the PMS delta Scuti star V351 Ori
V. Ripepi; M. Marconi; S. Bernabei; F. Palla; F. J. G. Pinheiro; D. F. M. Folha; T.D. Oswalt; L. Terranegra; A. Arellano Ferro; X.J. Jiang; J.M. Alcalá; S. Marinoni; M.J.P.F.G. Monteiro; M. Rudkin; K. Johnston;
26 Jun 2003   /  Astron.Astrophys. 408 (2003) 1047-1056
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22.
Anomalous RR Lyrae stars(?). III. CM Leonis
L. Di Fabrizio; G. Clementini; M. Marconi; E. Carretta; I.I. Ivans; A. Bragaglia; S. Di Tomaso; R. Merighi; H.A. Smith; C. Sneden; M. Tosi;
2 Jul 2002   /  Mon.Not.Roy.Astron.Soc. 336 (2002) 841
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23.
Peering through the dust: Evidence for a supermassive Black Hole at the nucleus of Centaurus A from VLT IR spectroscopy
Alessandro Marconi; Alessandro Capetti; David Axon; Anton Koekemoer; Duccio Macchetto; Ethan Schreier;
2 Nov 2000
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24.
Pulsation and evolutionary masses of classical Cepheids. I. Milky Way variables
F. Caputo; G. Bono; G. Fiorentino; M. Marconi; I. Musella;
8 May 2005   /  Astrophys.J. 629 (2005) 1021-1033
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25.
The Distance to NGC 5904 (M 5) via the Subdwarfs Main Sequence Fitting Method
Vincenzo Testa; Alessandro Chieffi; Marco Limongi; Gloria Andreuzzi; Gianni Marconi;
11 Mar 2004   /  Astron.Astrophys. 421 (2004) 603-612
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26.
Classical Cepheid pulsation models. VI. The Hertzsprung progression
G. Bono; M. Marconi; R. F. Stellingwerf;
16 Jun 2000
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27.
Theoretical Models for Classical Cepheids: VII. Metallicity effects on the Cepheid distance scale
F. Caputo; M. Marconi; I. Musella; P. Santolamazza;
16 Jun 2000
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28.
Pulsational M_V versus [Fe/H] relation(s) for globular cluster RR Lyrae variables
F. Caputo; V. Castellani; M. Marconi; V. Ripepi;
31 Mar 2000   /  Mon.Not.Roy.Astron.Soc. 316 (2000) 819
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29.
The RR Lyrae U Com as a test for nonlinear pulsation models
G. Bono; V. Castellani; M. Marconi;
11 Feb 2000
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30.
Theoretical Models for Classical Cepheids: IV. Mean Magnitudes and Colors and the Evaluation of Distance, Reddening and Metallicity
F. Caputo; M. Marconi; V. Ripepi;
3 Jun 1999
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