Zobrazeno 1 - 10
of 75
pro vyhledávání: '"S. Pedicelli"'
Autor:
L. Ravà, D. Fintini, M. Mariani, A. Deodati, E. Inzaghi, S. Pedicelli, C. Bizzarri, M. Cappa, S. Cianfarani, M. Manco
Publikováno v:
Journal of Endocrinological Investigation.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb0247c9685f990eb875e9a3b2d1d0ca
https://doi.org/10.1007/s40618-023-02111-6
https://doi.org/10.1007/s40618-023-02111-6
Akademický článek
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Akademický článek
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Autor:
Martino Romaniello, Francesca Primas, R. da Silva, Laura Inno, Noriyuki Matsunaga, P. François, Bertrand Lemasle, Eva K. Grebel, V. V. Kovtyukh, Giuseppe Bono, J. Pritchard, Giuliana Fiorentino, Martin Groenewegen, S. Pedicelli
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 608, pp.A85. ⟨10.1051/0004-6361/201731370⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 608, pp.A85. ⟨10.1051/0004-6361/201731370⟩
Context: Cepheids are excellent tracers of young stellar populations. They play a crucial role in astrophysics as standard candles. The chemistry of classical Cepheids in the Milky Way is now quite well-known. Despite a much larger sample, the chemic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e49d168c7d95a000203329b6d5cd818d
http://hdl.handle.net/2108/241396
http://hdl.handle.net/2108/241396
Autor:
Marcella Marconi, S. Pedicelli, J. W. Pel, Giuseppe Bono, Roberto Molinaro, J. Lub, Vincenzo Ripepi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 413:942-956
We present a new derivation of the CORS Baade-Wesselink method in the Walraven photometric system. We solved the complete Baade-Wesselink equation by calibrating the surface brightness function with a recent grid of atmosphere models. The new approac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a7d05759deccfe4ce890f9b2563b1e0f
https://doi.org/10.1111/j.1365-2966.2010.18183.x
https://doi.org/10.1111/j.1365-2966.2010.18183.x
Autor:
R. Buonanno, Giuseppe Bono, D. Laney, J. Pritchard, Santi Cassisi, Filippina Caputo, A. M. Piersimoni, Bertrand Lemasle, S. Pedicelli, Martino Romaniello, J. W. Pel, Martin Groenewegen, Silvia Leurini, F. Castelli, Francesca Primas, A. Pietrinferni, P. François, J. Lub
Publikováno v:
Astronomy & astrophysics, 504(1), 81-86. EDP Sciences
Aims: The iron abundance gradient in the Galactic stellar disk provides fundamental constraints on the chemical evolution of this important Galaxy component. However the spread around the mean slope is, at fixed Galactocentric distance, larger than e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c0479571729a44edd8f324b710e5fc5
https://doi.org/10.1051/0004-6361/200912504
https://doi.org/10.1051/0004-6361/200912504
Autor:
Martino Romaniello, S. Pedicelli, Francesca Primas, C. D. Laney, A. M. Piersimoni, P. François, B. Lemasle, Giuseppe Bono
Publikováno v:
Astronomy & Astrophysics. 490:613-623
Context: Classical Cepheids can be adopted to trace the chemical evolution of the Galactic disk since their distances can be estimated with very high accuracy. Aims: Homogeneous iron abundance measurements for 33 Galactic Cepheids located in the oute
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cfd2814e2349e272bd5bdd36afe5375
https://doi.org/10.1051/0004-6361:200810192
https://doi.org/10.1051/0004-6361:200810192
Autor:
Giuseppe Bono, L. Pulone, G. Iannicola, C. E. Corsi, Merieme Chadid, Martino Romaniello, M. Monelli, P. B. Stetson, A. M. Piersimoni, R. Buonanno, Annalisa Calamida, Francesca Primas, S. Pedicelli, I. Ferraro
Publikováno v:
EAS Publications Series. 25:125-135
We discuss how a wide field imager with very high spatial resolution on a relatively small telescope–but located in an observing site with very good seeing–might constrain the fraction of binary stars in Galactic globular clusters. We also mentio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::43090fce04348109ef49119af42ffaef
https://doi.org/10.1051/eas:2007083
https://doi.org/10.1051/eas:2007083
Akademický článek
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Autor:
S. Pedicelli, B. Lemasle, Francesca Primas, Lex Kaper, Martino Romaniello, V. V. Kovtyukh, Maria Bergemann, K. Genovali, Laura Inno, M. Fabrizio, C. D. Laney, P. Francois, Noriyuki Matsunaga, Giuseppe Bono
Publikováno v:
Astronomy & astrophysics, 558:A31. EDP Sciences
Astronomy & Astrophysics, 558. EDP Sciences
Astronomy & Astrophysics, 558. EDP Sciences
Context: Galactic abundance gradients set strong constraints to chemo-dynamical evolutionary models of the Milky Way. Given the PL relations that provide accurate distances and the large number of spectral lines, Cepheids are excellent tracers of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68e2a2e87b8e2ec3ec11ffa0af75be56
http://adsabs.harvard.edu/abs/2013A&A...558A..31L
http://adsabs.harvard.edu/abs/2013A&A...558A..31L