Zobrazeno 1 - 10
of 39
pro vyhledávání: '"D. PRICOPI"'
Publikováno v:
INCAS Bulletin, Vol 16, Iss 1, Pp 25-31 (2024)
Our work utilizes the quantum model of the hydrogen atom which is based on the Schrödinger equation with Coulomb potential. Specifically, we concentrate on the angular components of the wave eigenfunctions derived from this model. We consider the qu
Externí odkaz:
https://doaj.org/article/3033f29a4c9a4898935d6661410ab65b
Autor:
Cristina C. Popescu, M. T. Rushton, Giovanni Natale, D. Pricopi, Ruizhi Yang, Jordan J. Thirlwall
We obtained an axi-symmetric model for the large-scale distribution of stars and dust in the Milky Way (MW) using a radiative transfer code that can account for the existing near-infrared (NIR)/mid-infrared/submm all-sky emission maps of our Galaxy.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2472bbaa0c292200cd177fe1ba1d4f81
Autor:
D. Pricopi, E. Popescu
Publikováno v:
Astrophysics and Space Science. 365
The Mucket-Treder-type potential was initially introduced to explain the discrepancy between Mercury’s observed perihelion advance and the computed value based on Newton’s law, but it can also be used for many astronomical situations as, for inst
Autor:
E. Popescu, D. Pricopi
Publikováno v:
Astrophysics and Space Science. 362
In this paper, we consider the generalized Buckingham potential. Using the McGehee’s regularizing transformations, we study the global flow for the two-body problem associated to this potential. By making vary the angular momentum constant in the t
Autor:
A. Miglio, C. Chiappini, B. Mosser, G. R. Davies, K. Freeman, L. Girardi, P. Jofré, D. Kawata, B. M. Rendle, M. Valentini, L. Casagrande, W. J. Chaplin, G. Gilmore, K. Hawkins, B. Holl, T. Appourchaux, K. Belkacem, D. Bossini, K. Brogaard, M.‐J. Goupil, J. Montalbán, A. Noels, F. Anders, T. Rodrigues, G. Piotto, D. Pollacco, H. Rauer, C. Allende Prieto, P. P. Avelino, C. Babusiaux, C. Barban, B. Barbuy, S. Basu, F. Baudin, O. Benomar, O. Bienaymé, J. Binney, J. Bland‐Hawthorn, A. Bressan, C. Cacciari, T. L. Campante, S. Cassisi, J. Christensen‐Dalsgaard, F. Combes, O. Creevey, M. S. Cunha, R. S. Jong, P. Laverny, S. Degl'Innocenti, S. Deheuvels, É. Depagne, J. Ridder, P. Di Matteo, M. P. Di Mauro, M.‐A. Dupret, P. Eggenberger, Y. Elsworth, B. Famaey, S. Feltzing, R. A. García, O. Gerhard, B. K. Gibson, L. Gizon, M. Haywood, R. Handberg, U. Heiter, S. Hekker, D. Huber, R. Ibata, D. Katz, S. D. Kawaler, H. Kjeldsen, D. W. Kurtz, N. Lagarde, Y. Lebreton, M. N. Lund, S. R. Majewski, P. Marigo, M. Martig, S. Mathur, I. Minchev, T. Morel, S. Ortolani, M. H. Pinsonneault, B. Plez, P. G. Prada Moroni, D. Pricopi, A. Recio‐Blanco, C. Reylé, A. Robin, I. W. Roxburgh, M. Salaris, B. X. Santiago, R. Schiavon, A. Serenelli, S. Sharma, V. Silva Aguirre, C. Soubiran, M. Steinmetz, D. Stello, K. G. Strassmeier, P. Ventura, R. Ventura, N. A. Walton, C. C. Worley
Publikováno v:
Astronomical Notes / Astronomische Nachrichten
Astronomical Notes / Astronomische Nachrichten, Wiley-VCH Verlag, 2017, 338 (6), pp.644-661. ⟨10.1002/asna.201713385⟩
Astronomical Notes / Astronomische Nachrichten, 2017, 338 (6), pp.644-661. ⟨10.1002/asna.201713385⟩
NASA Astrophysics Data System
Miglio, A, Chiappini, C, Mosser, B, Davies, G R, Freeman, K, Girardi, L, Jofre, P, Kawata, D, Rendle, B M, Valentini, M, Casagrande, L, Chaplin, W J, Gilmore, G, Hawkins, K, Holl, B, Appourchaux, T, Belkacem, K, Bossini, D, Brogaard, K, Goupil, M-J, Montalban, J, Noels, A, Anders, F, Rodrigues, T, Piotto, G, Pollacco, D, Rauer, H, Allende Prieto, C, Avelino, P P, Babusiaux, C, Barban, C, Barbuy, B, Basu, S, Baudin, F, Benomar, O, Bienayme, O, Binney, J, Bland-Hawthorn, J, Bressan, A, Cacciari, C, Campante, T L, Cassisi, S, Christensen-Dalsgaard, J, Combes, F, Creevey, O, Cunha, M S, de Jong, R S, de laverny, P, Degl'Innocenti, S, Deheuvels, S, Depagne, E, De Ridder, J, Di Matteo, P, Di Mauro, M P, Dupret, M-A, Eggenberger, P, Elsworth, Y, Famaey, B, Feltzing, S, Garcia, R A, Gerhard, O, Gibson, B K, Gizon, L, Haywood, M, Handberg, R, Heiter, U, Hekker, S, Huber, D, Ibata, R, Katz, D, Kawaler, S D, Kjeldsen, H, Kurtz, D W, Lagarde, N, Lebreton, Y, Lund, M N, Majewski, S R, Marigo, P, Martig, M, Mathur, S, Minchev, I, Morel, T, Ortolani, S, Pinsonneault, M H, Plez, B, Moroni, P G P, Pricopi, D, Recio-Blanco, A, Reyle, C, Robin, A, Roxburgh, I W, Salaris, M, Santiago, B X, Schiavon, R, Serenelli, A, Sharma, S, Aguirre, V S, Soubiran, C, Steinmetz, M, Stello, D, Strassmeier, K G, Ventura, P, Ventura, R, Walton, N A & Worley, C C 2017, ' PLATO as it is : A legacy mission for Galactic archaeology ', Astronomische Nachrichten, vol. 338, no. 6, pp. 644-661 . https://doi.org/10.1002/asna.201713385
Astronomical Notes / Astronomische Nachrichten, Wiley-VCH Verlag, 2017, 338 (6), pp.644-661. ⟨10.1002/asna.201713385⟩
Astronomical Notes / Astronomische Nachrichten, 2017, 338 (6), pp.644-661. ⟨10.1002/asna.201713385⟩
NASA Astrophysics Data System
Miglio, A, Chiappini, C, Mosser, B, Davies, G R, Freeman, K, Girardi, L, Jofre, P, Kawata, D, Rendle, B M, Valentini, M, Casagrande, L, Chaplin, W J, Gilmore, G, Hawkins, K, Holl, B, Appourchaux, T, Belkacem, K, Bossini, D, Brogaard, K, Goupil, M-J, Montalban, J, Noels, A, Anders, F, Rodrigues, T, Piotto, G, Pollacco, D, Rauer, H, Allende Prieto, C, Avelino, P P, Babusiaux, C, Barban, C, Barbuy, B, Basu, S, Baudin, F, Benomar, O, Bienayme, O, Binney, J, Bland-Hawthorn, J, Bressan, A, Cacciari, C, Campante, T L, Cassisi, S, Christensen-Dalsgaard, J, Combes, F, Creevey, O, Cunha, M S, de Jong, R S, de laverny, P, Degl'Innocenti, S, Deheuvels, S, Depagne, E, De Ridder, J, Di Matteo, P, Di Mauro, M P, Dupret, M-A, Eggenberger, P, Elsworth, Y, Famaey, B, Feltzing, S, Garcia, R A, Gerhard, O, Gibson, B K, Gizon, L, Haywood, M, Handberg, R, Heiter, U, Hekker, S, Huber, D, Ibata, R, Katz, D, Kawaler, S D, Kjeldsen, H, Kurtz, D W, Lagarde, N, Lebreton, Y, Lund, M N, Majewski, S R, Marigo, P, Martig, M, Mathur, S, Minchev, I, Morel, T, Ortolani, S, Pinsonneault, M H, Plez, B, Moroni, P G P, Pricopi, D, Recio-Blanco, A, Reyle, C, Robin, A, Roxburgh, I W, Salaris, M, Santiago, B X, Schiavon, R, Serenelli, A, Sharma, S, Aguirre, V S, Soubiran, C, Steinmetz, M, Stello, D, Strassmeier, K G, Ventura, P, Ventura, R, Walton, N A & Worley, C C 2017, ' PLATO as it is : A legacy mission for Galactic archaeology ', Astronomische Nachrichten, vol. 338, no. 6, pp. 644-661 . https://doi.org/10.1002/asna.201713385
Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy. Data from large-scale astrometric and spectroscopic surveys will soon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e5ef1452a5fe5228a2e2216756f4ec4
https://elib.dlr.de/116317/
https://elib.dlr.de/116317/
Autor:
D. Pricopi
Publikováno v:
Astrophysics and Space Science. 361
The famous Yukawa-type potential was very often used for explaining a great variety of recent observed astronomical phenomena which range from the solar-system scale to cosmological distances. In this paper we tackle the two-body problem in the Yukaw
Autor:
E. Popescu, D. Pricopi
Publikováno v:
Astrophysics and Space Science. 361
In this paper, we study the global flow for the two-body problem associated to the Buckingham potential. For this, using McGehee-type transformations, we write the regularized equations of motion. Then, reducing the 4-dimensional phase space to a 2-d
Autor:
Joanna Molenda-Żakowicz, S. Bernabei, L. A. Balona, Vincenzo Ripepi, A. Moya, D. Pricopi, Todd C. Klaus, Jadwiga Daszyńska-Daszkiewicz, Marcella Marconi, Giovanni Catanzaro, Victoria Antoci, Karen Kinemuchi, A. Grigahcène, M. Di Criscienzo, J. C. Suárez, M. D. Suran, Patrick Lenz, Barry Smalley, Andrzej Pigulski, Gerald Handler, D. W. Kurtz, J. M. Nemec, Jennifer R. Hall
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 419:3028-3038
We analyse Kepler observations of the high-amplitude δ Scuti (HADS) star V2367 Cyg (KIC 9408694). The variations are dominated by a mode with frequency f1= 5.6611 d−1. Two other independent modes with f2= 7.1490 d−1 and f3= 7.7756 d−1 have amp
Autor:
L. A. Balona, A. Pigulski, P. De Cat, G. Handler, J. Gutiérrez-Soto, C. A. Engelbrecht, F. Frescura, M. Briquet, J. Cuypers, J. Daszyńska-Daszkiewicz, P. Degroote, R. J. Dukes, R. A. Garcia, E. M. Green, U. Heber, S. D. Kawaler, H. Lehmann, B. Leroy, J. Molenda-Żakowicz, C. Neiner, A. Noels, J. Nuspl, R. Østensen, D. Pricopi, I. Roxburgh, S. Salmon, M. A. Smith, J. C. Suárez, M. Suran, R. Szabó, K. Uytterhoeven, null Christensen-Dalsgaard, H. Kjeldsen, D. A. Caldwell, F. R. Girouard, D. T. Sanderfer
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 413:2403-2420
The analysis of the light curves of 48 B-type stars observed by Kepler is presented. Among these are 15 pulsating stars, all of which show low frequencies characteristic of SPB stars. Seven of these stars also show a few weak, isolated high frequenci
Autor:
D. Pricopi, M. D. Suran
Publikováno v:
Communications in Asteroseismology. 153:28-34
In this paper, we report our preliminary results regarding the asteroseismic modeling of the slow pulsating B star HD 163830, based on eighteen of the twenty detected frequencies of this star. The powerful method of matching stellar models both to os