Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Chorniy, Y"'
Autor:
Tautvaišienė, G., Mikolaitis, Š., Drazdauskas, A., Stonkutė, E., Minkevičiūtė, R., Pakštienė, E., Kjeldsen, H., Brogaard, K., Chorniy, Y., von Essen, C., Grundahl, F., Ambrosch, M., Bagdonas, V., Sharma, A., Vázquez, C. Viscasillas
In fulfilling the aims of the planetary and asteroseismic research missions, such as that of the NASA Transiting Exoplanet Survey Satellite (TESS) space telescope, accurate stellar atmospheric parameters and a detailed chemical composition are requir
Externí odkaz:
http://arxiv.org/abs/2202.10102
Autor:
Tautvaisiene, G., Drazdauskas, A., Bragaglia, A., Martell, S. L., Pancino, E., Lardo, C., Mikolaitis, S., Minkeviciute, R., Stonkute, E., Ambrosch, M., Bagdonas, V., Chorniy, Y., Sanna, N., Franciosini, E., Smiljanic, R., Randich, S., Gilmore, G., Bensby, T., Bergemann, M., Gonneau, A., Guiglion, G., Carraro, G., Heiter, U., Korn, A., Magrini, L., Morbidelli, L., Zaggia, S.
Publikováno v:
A&A 658, A80 (2022)
Context. NGC 1851 is one of several globular clusters for which multiple stellar populations of the subgiant branch have been clearly identified and a difference in metallicity detected. A crucial piece of information on the formation history of this
Externí odkaz:
http://arxiv.org/abs/2111.10684
Autor:
Casali, G., Magrini, L., Tognelli, E., Jackson, R., Jeffries, R. D., Lagarde, N., Tautvaisiene, G., Masseron, T., Degl'Innocenti, S., Moroni, P. G. Prada, Kordopatis, G., Pancino, E., Randich, S., Feltzing, S., Sahlholdt, C., Spina, L., Friel, E., Roccatagliata, V., Sanna, N., Bragaglia, A., Drazdauskas, A., Mikolaitis, S., Minkeviciute, R., Stonkute, E., Chorniy, Y., Bagdonas, V., Jimenez-Esteban, F., Martell, S., Van der Swaelmen, M., Gilmore, G., Vallenari, A., Bensby, T., Koposov, S. E., Korn, A., Worley, C., Smiljanic, R., Bergemann, M., Carraro, G., Damiani, F., Prisinzano, L., Bonito, R., Franciosini, E., Gonneau, A., Hourihane, A., Jofre, P., Lewis, J., Morbidelli, L., Sacco, G., Sousa, S. G., Zaggia, S., Lanzafame, A. C., Heiter, U., Frasca, A., Bayo, A.
Publikováno v:
A&A 629, A62 (2019)
In the era of large high-resolution spectroscopic surveys, high-quality spectra can contribute to our understanding of the Galactic chemical evolution, providing chemical abundances belonging to the different nucleosynthesis channels, and also provid
Externí odkaz:
http://arxiv.org/abs/1907.07350
Autor:
Magrini, L., Vincenzo, F., Randich, S., Pancino, E., Casali, G., Tautvaisiene, G., Drazdauskas, A., Mikolaitis, S., Minkeviciute, R., Stonkute, E., Chorniy, Y., Bagdonas, V., Kordopatis, G., Frie, E., Roccatagliata, V., Jimenez-Esteban, F. M., Gilmore, G., Vallenari, A., Bensby, T., Bragaglia, A., Korn, A. J., Lanzafame, A. C., Smiljanic, R., Bayo, A., Casey, A. R., Costado, M. T., Franciosini, E., Hourihane, A., Jofré, Lewis, J., Monaco, L., Morbidelli, L., Sacco, G., Worley, C.
Publikováno v:
A&A 618, A102 (2018)
The abundance ratio N/O is a useful tool to study the interplay of galactic processes, e.g. star formation efficiency, time-scale of infall and outflow loading factor We aim to trace log(N/O) versus [Fe/H] in the Milky Way and to compare it with a se
Externí odkaz:
http://arxiv.org/abs/1807.06297
Autor:
Lagarde, N., Reylé, C., Robin, A. C., Tautvaišienė, G., Drazdauskas, A., Mikolaitis, Š., Minkevičiūtė, R., Stonkutė, E., Chorniy, Y., Bagdonas, V., Miglio, A., Nasello, G., Gilmore, G., Randich, S., Bensby, T., Bragaglia, A., Flaccomio, E., Francois, P., Korn, A. J., Pancino, E., Smiljanic, R., Bayo, A., Carraro, G., Costado, M. T., Jiménez-Esteban, F., Jofré, P., Martell, S. L., Masseron, T., Monaco, L., Morbidelli, L., Sbordone, L., Sousa, S. G., Zaggia, S.
Publikováno v:
A&A 621, A24 (2019)
The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical elements C and N at their surface. The surface abundances of these chem
Externí odkaz:
http://arxiv.org/abs/1806.01868
Autor:
Fu, Xiaoting., Romano, D., Bragaglia, A., Mucciarelli, A., Lind, K., Mena, E. Delgado, Sousa, S. G., Randich, S., Bressan, A., Sbordone, L., Martell, S., Korn, A. J., Abia, C., Smiljanic, R., Jofré, P., Pancino, E., Tautvaišienė, G., Tang, B., Magrini, L., Lanzafame, A. C., Carraro, G., Bensby, T., Damiani, F., Alfaro, E. J., Flaccomio, E., Morbidelli, L., Zaggia, S., Lardo, C., Monaco, L., Frasca, A., Donati, P., Drazdauskas, A., Chorniy, Y., Bayo, A., Kordopatis, G.
Publikováno v:
A&A 610, A38 (2018)
Lithium abundance in most of the warm metal-poor main sequence stars shows a constant plateau (A(Li)~2.2 dex) and then the upper envelope of the lithium vs. metallicity distribution increases as we approach solar metallicity. Meteorites, which carry
Externí odkaz:
http://arxiv.org/abs/1711.04829
Autor:
Casey, A. R., Ruchti, G., Masseron, T., Randich, S., Gilmore, G., Lind, K., Kennedy, G. M., Koposov, S. E., Hourihane, A., Franciosini, E., Lewis, J. R., Magrini, L., Morbidelli, L., Sacco, G. G., Worley, C. C., Feltzing, S., Jeffries, R. D., Vallenari, A., Bensby, T., Bragaglia, A., Flaccomio, E., Francois, P., Korn, A. J., Lanzafame, A., Pancino, E., Recio-Blanco, A., Smiljanic, R., Carraro, G., Costado, M. T., Damiani, F., Donati, P., Frasca, A., Jofré, P., Lardo, C., de Laverny, P., Monaco, L., Prisinzano, L., Sbordone, L., Sousa, S. G., Tautvaišienė, G., Zaggia, S., Zwitter, T., Mena, E. Delgado, Chorniy, Y., Martell, S. L., Aguirre, V. Silva, Miglio, A., Chiappini, C., Montalban, J., Morel, T., Valentini, M.
The discovery of lithium-rich giants contradicts expectations from canonical stellar evolution. Here we report on the serendipitous discovery of 20 Li-rich giants observed during the Gaia-ESO Survey, which includes the first nine Li-rich giant stars
Externí odkaz:
http://arxiv.org/abs/1603.03038
Autor:
Tautvaišienė, G., Drazdauskas, A., Mikolaitis, Š., Barisevičius, G., Puzeras, E., Stonkutė, E., Chorniy, Y., Magrini, L., Romano, D., Smiljanic, R., Bragaglia, A., Carraro, G., Friel, E., Morel, T., Pancino, E., Donati, P., Jiménez-Esteban, F., Gilmore, G., Randich, S., Jeffries, R. D., Vallenari, A., Bensby, T., Flaccomio, E., Recio-Blanco, A., Costado, M. T., Hill, V., Jofré, P., Lardo, C., de Laverny, P., Masseron, T., Moribelli, L., Sousa, S. G., Zaggia, S.
Aim of this work is to determine C, N, and O abundances in stars of Galactic open clusters of the Gaia-ESO survey and to compare the observed abundances with those predicted by current stellar and Galactic evolution models. In this pilot paper, we in
Externí odkaz:
http://arxiv.org/abs/1411.2831
Autor:
Smiljanic, R., Korn, A. J., Bergemann, M., Frasca, A., Magrini, L., Masseron, T., Pancino, E., Ruchti, G., Roman, I. San, Sbordone, L., Sousa, S. G., Tabernero, H., Tautvaisiene, G., Valentini, M., Weber, M., Worley, C. C., Adibekyan, V. Zh., Prieto, C. Allende, Barisevicius, G., Biazzo, K., Blanco-Cuaresma, S., Bonifacio, P., Bragaglia, A., Caffau, E., Cantat-Gaudin, T., Chorniy, Y., de Laverny, P., Delgado-Mena, E., Donati, P., Duffau, S., Franciosini, E., Friel, E., Geisler, D., Hernandez, J. I. Gonzalez, Gruyters, P., Guiglion, G., Hansen, C. J., Heiter, U., Hill, V., Jacobson, H. R., Jofre, P., Jonsson, H., Lanzafame, A. C., Lardo, C., Ludwig, H. G., Maiorca, E., Mikolaitis, S., Montes, D., Morel, T., Mucciarelli, A., Munoz, C., Nordlander, T., Pasquini, L., Puzeras, E., Recio-Blanco, A., Ryde, N., Sacco, G., Santos, N. C., Serenelli, A. M., Sordo, R., Soubiran, C., Spina, L., Steffen, M., Vallenari, A., Van Eck, S., Villanova, S., Gilmore, G., Randich, S., Asplund, M., Binney, J., Drew, J., Feltzing, S., Ferguson, A., Jeffries, R., Micela, G., Negueruela, I., Prusti, T., Rix, H-W., Alfaro, E., Babusiaux, C., Bensby, T., Blomme, R., Flaccomio, E., Francois, P., Irwin, M., Koposov, S., Walton, N., Bayo, A., Carraro, G., Costado, M. T., Damiani, F., Edvardsson, B., Hourihane, A., Jackson, R., Lewis, J., Lind, K., Marconi, G., Martayan, C., Monaco, L., Morbidelli, L., Prisinzano, L., Zaggia, S.
Publikováno v:
A&A 570, A122 (2014)
The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-type stars. These UVES spectra are analyzed in parallel by several stat
Externí odkaz:
http://arxiv.org/abs/1409.0568
In this work we present the main atmospheric parameters, carbon, nitrogen and oxygen abundances, and 12C/13C ratios determined in a sample of 28 Galactic clump stars. Abundances of carbon were studied using the C2 band at 5086.2 {\AA}. The wavelength
Externí odkaz:
http://arxiv.org/abs/1304.4393