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of 5
pro vyhledávání: '"Duarte, Tharcísyo"'
Autor:
Duarte, Tharcisyo S? e Sousa
Publikováno v:
Repositório Institucional da UFRNUniversidade Federal do Rio Grande do NorteUFRN.
Submitted by Automa??o e Estat?stica (sst@bczm.ufrn.br) on 2017-03-09T19:50:49Z No. of bitstreams: 1 TharcisyoSaESousaDuarte_TESE.pdf: 4000536 bytes, checksum: 76f14cacb9f32138dca1e02cb150ad3b (MD5)
Approved for entry into archive by Arlan Eloi
Approved for entry into archive by Arlan Eloi
Externí odkaz:
https://repositorio.ufrn.br/jspui/handle/123456789/22221
Autor:
Duarte, Tharcisyo Sa e Sousa
Publikováno v:
Repositório Institucional da UFRNUniversidade Federal do Rio Grande do NorteUFRN.
Made available in DSpace on 2015-03-03T15:15:27Z (GMT). No. of bitstreams: 1 TharcisyoSSD_DISSERT.pdf: 3303211 bytes, checksum: cec9a1421d7e1a74109ea2385531baa3 (MD5) Previous issue date: 2012-03-02
This study proposes an observing program focus
This study proposes an observing program focus
Externí odkaz:
http://repositorio.ufrn.br:8080/jspui/handle/123456789/18597
Autor:
De Moura, Bruno Lustosa, Beck, Paul G., de Almeida, Leandro, Duarte, Tharcisyo S. S., Coelho, Hugo R., da Costa, Jefferson S., Castro, Matthieu, Nascimento Jr, Jose-Dias do
Publikováno v:
The Astrophysical Journal, Volume 894, Number 1, 2020
In order to clarify the properties of the secondary clump star HD 226808 (KIC 5307747), we combined four years of data from Kepler space photometry with high-resolution spectroscopy of the High Efficiency and Resolution Mercator \'Echelle Spectrograp
Externí odkaz:
http://arxiv.org/abs/2005.03140
Publikováno v:
A&A 590, A94 (2016)
Lithium abundances in open clusters provide an effective way of probing mixing processes in the interior of solar-type stars and convection is not the only mixing mechanism at work. To understand which mixing mechanisms are occurring in low-mass star
Externí odkaz:
http://arxiv.org/abs/1603.08809
Magnetic fields of late-type stars are presumably generated by a dynamo mechanism at the interface layer between the radiative interior and the outer convective zone. The Rossby number, which is related to the dynamo process, shows an observational c
Externí odkaz:
http://arxiv.org/abs/1309.7974