Zobrazeno 1 - 10
of 90
pro vyhledávání: '"Ramos, R Contreras"'
Autor:
Albarracín, Rogelio, Zoccali, M., Carvajal, J. Olivares, Rojas-Arriagada, Á., Minniti, J. H., Catelan, M., De Leo, M., Gran, F., Ramos, R. Contreras, Navarro, Á. Valenzuela, Salvo-Guajardo, C.
Publikováno v:
A&A 693, A28 (2025)
The structure and kinematics of the Milky Way disk are largely inferred from the solar vicinity. To gain a comprehensive understanding, it is essential to find reliable tracers in less-explored regions like the bulge and the far side of the disk. Mir
Externí odkaz:
http://arxiv.org/abs/2411.04623
Autor:
Ordenes-Huanca, C., Zoccali, M., Bayo, A., Cuadra, J., Ramos, R. Contreras, Rojas-Arriagada, A.
NGC 6357, a star-forming complex at $\sim 1.7$ kpc from the Sun, contains giant molecular clouds and three prominent star clusters alongside with HII regions, very massive stars and thousands of young stellar objects in different evolutionary stages.
Externí odkaz:
http://arxiv.org/abs/2407.17577
Autor:
Zoccali, M., Quezada, C., Ramos, R. Contreras, Valenti, E., Valenzuela-Navarro, A., Carvajal, J. Olivares, Arriagada, A. Rojas, Minniti, J. H., Gran, F., De Leo, M.
Publikováno v:
A&A 689, A240 (2024)
Context. Observational evidence has accumulated in the past years, showing that the Galactic bulge includes two populations, a metal poor and a metal rich one that, in addition to a different metallicity, show different alpha over iron abundances, sp
Externí odkaz:
http://arxiv.org/abs/2407.11226
Autor:
Saito, R. K., Hempel, M., Alonso-García, J., Lucas, P. W., Minniti, D., Alonso, S., Baravalle, L., Borissova, J., Caceres, C., Chené, A. N., Cross, N. J. G., Duplancic, F., Garro, E. R., Gómez, M., Ivanov, V. D., Kurtev, R., Luna, A., Majaess, D., Navarro, M. G., Pullen, J. B., Rejkuba, M., Sanders, J. L., Smith, L. C., Albino, P. H. C., Alonso, M. V., Amôres, E. B., Angeloni, R., Arias, J. I., Arnaboldi, M., Barbuy, B., Bayo, A., Beamin, J. C., Bedin, L. R., Bellini, A., Benjamin, R. A., Bica, E., Bonatto, C. J., Botan, E., Braga, V. F., Brown, D. A., Cabral, J. B., Camargo, D., Garatti, A. Caratti o, Carballo-Bello, J. A., Catelan, M., Chavero, C., Chijani, M. A., Clariá, J. J., Coldwell, G. V., Peña, C. Contreras, Ramos, R. Contreras, Corral-Santana, J. M., Cortés, C. C., Cortés-Contreras, M., Cruz, P., Daza-Perilla, I. V., Debattista, V. P., Dias, B., Donoso, L., D'Souza, R., Emerson, J. P., Federle, S., Fermiano, V., Fernandez, J., Fernández-Trincado, J. G., Ferreira, T., Lopes, C. E. Ferreira, Firpo, V., Flores-Quintana, C., Fraga, L., Froebrich, D., Galdeano, D., Gavignaud, I., Geisler, D., Gerhard, O. E., Gieren, W., Gonzalez, O. A., Gramajo, L. V., Gran, F., Granitto, P. M., Griggio, M., Guo, Z., Gurovich, S., Hilker, M., Jones, H. R. A., Kammers, R., Kuhn, M. A., Kumar, M. S . N., Kundu, R., Lares, M., Libralato, M., Lima, E., Maccarone, T. J., Cortés, P. Marchant, Martin, E. L., Masetti, N., Matsunaga, N., Mauro, F., McDonald, I., Mejías, A., Mesa, V., Milla-Castro, F. P., Minniti, J. H., Bidin, C. Moni, Montenegro, K., Morris, C., Motta, V., Navarete, F., Molina, C. Navarro, Nikzat, F., Castellón, J. L. Nilo, Obasi, C., Ortigoza-Urdaneta, M., Palma, T., Parisi, C., Ramírez, K. Pena, Pereyra, L., Perez, N., Petralia, I., Pichel, A., Pignata, G., Alegría, S. Ramírez, Rojas, A. F., Rojas, D., Roman-Lopes, A., Rovero, A. C., Saroon, S., Schmidt, E. O., Schröder, A. C., Schultheis, M., Sgró, M. A., Solano, E., Soto, M., Stecklum, B., Steeghs, D., Tamura, M., Tissera, P., Valcarce, A. A. R., Valotto, C. A., Vasquez, S., Villalon, C., Villanova, S., Cádiz, F. Vivanco, Bacigalupo, R. Zelada, Zijlstra, A., Zoccali, M.
Publikováno v:
A&A 689, A148 (2024)
The ESO public survey VISTA Variables in the V\'ia L\'actea (VVV) surveyed the inner Galactic bulge and the adjacent southern Galactic disk from $2009-2015$. Upon its conclusion, the complementary VVV eXtended (VVVX) survey has expanded both the temp
Externí odkaz:
http://arxiv.org/abs/2406.16646
Autor:
Carvajal, J. Olivares, Zoccali, M., De Leo, M., Ramos, R. Contreras, Quezada, C., Rojas-Arriagada, Á., Valenti, E., Albarracín, R., Navarro, Á. Valenzuela
Publikováno v:
A&A 687, A312 (2024)
The structure and kinematics of the old component of the Galactic bulge are still a matter of debate. The bulk of the bulge as traced by red clump stars includes two main components, which are usually identified as the metal-rich and metal-poor compo
Externí odkaz:
http://arxiv.org/abs/2405.08990
Autor:
Zoccali, M., Rojas-Arriagada, A., Valenti, E., Ramos, R. Contreras, Valenzuela-Navarro, A., Salvo-Guajardo, C.
The nuclear region of the Milky Way is believed to host a nuclear stellar disk, co-spatial with the gaseous central molecular zone. Previous kinematical studies detected faster rotation for the stars belonging to the nuclear stellar disk, compared to
Externí odkaz:
http://arxiv.org/abs/2402.16800
Autor:
Gran, F., Kordopatis, G., Zoccali, M., Hill, V., Saviane, I., Navarrete, C., Rojas-Arriagada, A., Carballo-Bello, J., Hartke, J., Valenti, E., Ramos, R. Contreras, De Leo, M., Fabbro, S.
After the second data release of Gaia, the number of new globular cluster candidates has increased importantly. However, most of them need to be properly characterised, both spectroscopically and photometrically, by means of radial velocities, metall
Externí odkaz:
http://arxiv.org/abs/2310.09868
Autor:
Ordenes-Huanca, C., Zoccali, M., Bayo, A., Cuadra, J., Ramos, R. Contreras, Hillenbrand, L. A., Lacerna, I., Abarzua, S., Avendaño, C., Diaz, P., Fernandez, I., Lara, G.
T Tauri stars are low-mass pre-main sequence stars that are intrinsically variable. Due to the intense magnetic fields they possess, they develop dark spots on their surface that, because of rotation, introduce a periodic variation of brightness.In a
Externí odkaz:
http://arxiv.org/abs/2210.09242
Autor:
Nikzat, F., Lopes, C. E. Ferreira, Catelan, M., Ramos, R. Contreras, Zoccali, M., Rojas-Arriagada, A., Braga, V. F., Minniti, D., Borissova, J., Becker, I.
Publikováno v:
A&A 660, A35 (2022)
Long-period variable stars (LPVs) are pulsating red giants, primarily in the asymptotic giant branch phase, and they include both Miras and semi-regular variables (SRVs). Their period-age and period-luminosity relations enable us to trace different s
Externí odkaz:
http://arxiv.org/abs/2203.06162
Autor:
Gran, F., Zoccali, M., Saviane, I., Valenti, E., Rojas-Arriagada, A., Ramos, R. Contreras, Hartke, J., Carballo-Bello, J. A., Navarrete, C., Rejkuba, M., Carvajal, J. Olivares
Recent wide-area surveys have enabled us to study the Milky Way with unprecedented detail. Its inner regions, hidden behind dust and gas, have been partially unveiled with the arrival of near-IR photometric and spectroscopic datasets. Among recent di
Externí odkaz:
http://arxiv.org/abs/2108.11922