Zobrazeno 1 - 7
of 7
pro vyhledávání: '"O. J. Katime Santrich"'
Autor:
B Dias, M C Parisi, M Angelo, F Maia, R A P Oliveira, S O Souza, L O Kerber, J F C Santos, A Pérez-Villegas, D Sanmartim, B Quint, L Fraga, B Barbuy, E Bica, O J Katime Santrich, J A Hernandez-Jimenez, D Geisler, D Minniti, B J De Bórtoli, L P Bassino, J P Rocha
The structure of the Small Magellanic Cloud (SMC) is very complex, in particular in the periphery that suffers more from the interactions with the Large Magellanic Cloud (LMC). A wealth of observational evidence has been accumulated revealing tidal t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d8b3f9c5d46fb69601950e9148cd4a3
http://arxiv.org/abs/2201.11119
http://arxiv.org/abs/2201.11119
Autor:
O. J. Katime Santrich, Bruno Quint, Bruno Dias, Pieter Westera, Lilia Patricia Bassino, Susana O. Souza, B. J. De Bortoli, R. A. P. Oliveira, F. F. S. Maia, Beatriz Barbuy, Angeles Pérez-Villegas, M. C. Parisi, D. Sanmartim, Doug Geisler, M. S. Angelo, Leandro Kerber, J. F. C. Santos, Eduardo Luiz Damiani Bica
Publikováno v:
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Context. The interactions between the SMC and LMC created the Magellanic Bridge, a stream of gas and stars pulled out of the SMC towards the LMC about 150 Myr ago. The tidal counterpart of this structure, which should include a trailing arm, has been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::098371fb799e4ae4b030bc5e2ddc3264
https://doi.org/10.1051/0004-6361/202040015
https://doi.org/10.1051/0004-6361/202040015
Publikováno v:
The Astrophysical Journal. 854:184
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b64b832a79fc72b6c397812c9dd3b7e5
https://doi.org/10.3847/1538-4357/aaa017
https://doi.org/10.3847/1538-4357/aaa017
Context: Open clusters are very useful targets for examining possible trends in galactocentric distance and age, especially when young and old open clusters are compared. Aims: We carried out a detailed spectroscopic analysis to derive the chemical c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47889c947d64521f6d4658fe05c94224
http://arxiv.org/abs/1304.1004
http://arxiv.org/abs/1304.1004
Autor:
C. B. Pereira, Fernando Roig, J. V. Sales Silva, V. J. Peña Suárez, O. J. Katime Santrich, Natalia A. Drake
Publikováno v:
The Astronomical Journal. 148:83
Binary stars in open clusters are very useful targets in constraining the nucleosynthesis process. The luminosities of the stars are known because the distances of the clusters are also known, so chemical peculiarities can be linked directly to the e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::015289b9f314cd98768c0b5b987e647b
https://doi.org/10.1088/0004-6256/148/5/83
https://doi.org/10.1088/0004-6256/148/5/83
Publikováno v:
The Astronomical Journal. 146:39
Open clusters are very useful examples to explain the constraint of the nucleosynthesis process with the luminosities of stars because the distances of the clusters are better known than those of field stars. We carried out a detailed spectroscopic a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f7ffe14e6186508239bddf0e5f1cb2a4
https://doi.org/10.1088/0004-6256/146/2/39
https://doi.org/10.1088/0004-6256/146/2/39
Publikováno v:
Astrophysical Journal; 2/20/2018, Vol. 854 Issue 2, p1-1, 1p