Zobrazeno 1 - 10
of 1 232
pro vyhledávání: '"Mello, C"'
Autor:
Razavi-Shearer, D., Child, H., Razavi-Shearer, K., Voeller, A., Razavi, H., Buti, M., Tacke, F., Terrault, N., Zeuzem, S., Abbas, Z., Aghemo, A., Akarca, U.S., Al Masri, N., Alalwan, A., Blomé, M. Alanko, Jerkeman, A., Aleman, S., Kamal, H., Alghamdi, A., Alghamdi, M., Alghamdi, S., Al-Hamoudi, W., Ali, E., Aljumah, A., Altraif, I., Amarsanaa, J., Asselah, T., Baatarkhuu, O., Babameto, A., Ben-Ari, Z., Berg, T., Biondi, M., Braga, W., Brandão-Mello, C., Brown, R., Brunetto, M., Cabezas, J., Cardoso, M., Martins, A., Chan, H.L.Y., Cheinquer, H., Chen, C.-J., Yang, H.-I., Chen, P.-J., Chien, C.-H., Chuang, W.-L., Garza, L. Cisneros, Coco, B., Coffin, C., Coppola, N., Cornberg, M., Craxi, A., Crespo, J., Cuko, L., De Ledinghen, V., Duberg, A.-S., Etzion, O., Ferraz, M.L., Ferreira, P., Forns, X., Foster, G., Fung, J., Gaeta, G., García-Samaniego, J., Genov, J., Gheorghe, L., Gholam, P., Gish, R., Glenn, J., Hamid, S., Hercun, J., Hsu, Y.-C., Hu, C.-C., Huang, J.-F., Idilman, R., Jafri, W., Janjua, N., Jelev, D., Jia, J., Kåberg, M., Kaita, K., Kao, J.-H., Khan, A., Kim, D.Y., Kondili, L., Lagging, M., Lampertico, P., Lázaro, P., Lazarus, J.V., Lee, M.-H., Lim, Y.-S., Lobato, C., Macedo, G., Marinho, R., Marotta, P., Mendes-Correa, M.C., Méndez-Sánchez, N., Navas, M.-C., Ning, Q., Örmeci, N., Orrego, M., Osiowy, C., Pan, C., Pessoa, M., Piracha, Z., Pop, C., Qureshi, H., Raimondo, G., Ramji, A., Ribeiro, S., Ríos-Hincapié, C., Rodríguez, M., Rosenberg, W., Roulot, D., Ryder, S., Saeed, U., Safadi, R., Shouval, D., Sanai, F., Sanchez-Avila, J.F., Santantonio, T., Sarrazin, C., Seto, W.-K., Simonova, M., Tanaka, J., Tergast, T., Tsendsuren, O., Valente, C., Villalobos-Salcedo, J.M., Waheed, Y., Wong, G., Wong, V., Yip, T., Wu, J.-C., Yu, M.-L., Yuen, M.-F., Yurdaydin, C., Zuckerman, E.
Publikováno v:
In Journal of Hepatology February 2024 80(2):232-242
Publikováno v:
A&A 616, A18 (2018)
Globular clusters are tracers of the history of star formation and chemical enrichment in the early Galaxy. Their abundance pattern can help understanding their chemical enrichment processes. In particular, the iron-peak elements have been relatively
Externí odkaz:
http://arxiv.org/abs/1801.06157
Autor:
Siqueira-Mello, C., Chiappini, C., Barbuy, B., Freeman, K., Ness, M., Depagne, E., Cantelli, E., Pignatari, M., Hirschi, R., Frischknecht, U., Meynet, G., Maeder, A.
Publikováno v:
A&A 593, A79 (2016)
Context. Efforts to look for signatures of the first stars have concentrated on metal-poor halo objects. However, the low end of the bulge metallicity distribution has been shown to host some of the oldest objects in the Milky Way and hence this Gala
Externí odkaz:
http://arxiv.org/abs/1605.08939
Autor:
Barbuy, B., Cantelli, E., Vemado, A., Ernandes, H., Ortolani, S., Saviane, I., Bica, E., Minniti, D., Dias, B., Momany, Y., Hill, V., Zoccali, M., Siqueira-Mello, C.
The globular cluster HP~1 is projected at only 3.33 degrees from the Galactic center. Together with its distance, this makes it one of the most central globular clusters in the Milky Way. It has a blue horizontal branch (BHB) and a metallicity of [Fe
Externí odkaz:
http://arxiv.org/abs/1604.02095
Publikováno v:
A&A 584, A86 (2015)
HD 140283 is a reference subgiant that is metal poor and confirmed to be a very old star. The abundances of this type of old star can constrain the nature and nucleosynthesis processes that occurred in its (even older) progenitors. The present study
Externí odkaz:
http://arxiv.org/abs/1509.00658
Autor:
Siqueira-Mello, C., Hill, V., Barbuy, B., Spite, M., Spite, F., Beers, T. C., Caffau, E., Bonifacio, P., Cayrel, R., François, P., Schatz, H., Wanajo, S.
Moderately r-process-enriched stars (r-I) are at least four times as common as those that are greatly enriched in r-process elements (r-II), and the abundances in their atmospheres are important tools for obtaining a better understanding of the nucle
Externí odkaz:
http://arxiv.org/abs/1404.0234
Autor:
Mello, C. Siqueira, Spite, M., Barbuy, B., Spite, F., Caffau, E., Hill, V., Wanajo, S., Primas, F., Plez, B., Cayrel, R., Andersen, J., Nordström, B., Sneden, C., Beers, T. C., Bonifacio, P., François, P., Molaro, P.
Detailed abundances of the elements produced by r-process nucleosynthesis in various circumstances are our best observational clues to their origin, since the site(s) of r-element production is(are) still not known with certainty. A small fraction of
Externí odkaz:
http://arxiv.org/abs/1212.0211
HD 140283 is a nearby (V=7.7) subgiant metal-poor star, extensively analysed in the literature. Although many spectra have been obtained for this star, none showed a signal-to-noise (S/N) ratio high enough to enable a very accurate derivation of abun
Externí odkaz:
http://arxiv.org/abs/1211.0693
Autor:
Alencar, J.1 (AUTHOR) jalencar@ioc.fiocruz.br, Ferreira de Mello, C.1,2 (AUTHOR), Silva, S. O. F.1,3 (AUTHOR), Guimarães, A. É.1 (AUTHOR), Müller, G. A.4 (AUTHOR)
Publikováno v:
European Zoological Journal. Dec2022, Vol. 89 Issue 1, p1018-1025. 8p.
Autor:
Souza, F. A., Carlin, N., Beck, C., Keeley, N., Diaz-Torres, A., Neto, R. Liguori, Siqueira-Mello, C., de Moura, M. M., Munhoz, M. G., Oliveira, R. A. N., Del Santo, M. G., Suade, A. A. P., Szanto, E. M., de Toledo, A. Szanto
Publikováno v:
Nucl.Phys.A834:420c-423c,2010
alpha-d coincidence data were studied for the 6Li + 59Co reaction at E(lab) = 29.6 MeV. By using a kinematic analysis, it was possible to identify which process, leading to the same final state, has the major contribution for each of the selected ang
Externí odkaz:
http://arxiv.org/abs/0910.0342