Zobrazeno 1 - 10
of 300
pro vyhledávání: '"Anguiano B"'
Autor:
Gonzalez-Torres MA, Salazar MA, Imaz M, Inchausti L, Ibañez B, Fernandez-Rivas A, Pastor J, Anguiano B, Muñoz P, Ruiz E, Oraa R, Bustamante S, Alvarez de Eulate S, Cisterna R
Publikováno v:
Neuropsychiatric Disease and Treatment, Vol 2015, Iss default, Pp 1421-1426 (2015)
Miguel Angel Gonzalez-Torres,1,2 Miguel Angel Salazar,3 Manuel Imaz,4 Lucía Inchausti,1,2 Berta Ibañez,5 Aranzazu Fernandez-Rivas,1,2 Javier Pastor,3 Bosco Anguiano,3 Pedro Muñoz,3 Eduardo Ruiz,1,2 Rodrigo Oraa,3 Sonia Bustamante,1,2 Sofia Alvarez
Externí odkaz:
https://doaj.org/article/d7e3e977e87245bcba7c10dcac9d2a13
Publikováno v:
EPJ Web of Conferences, Vol 19, p 05009 (2012)
We present preliminary results from follow-up observations of a carefully selected sample of subgiant stars from RAVE and Geneva-Copenhagen surveys. We find evidence of rapid saturation of the heating mechanism in the disk, with an abrupt increase of
Externí odkaz:
https://doaj.org/article/f6c8960d63cc4d7cbe35f41cc73c9df2
Autor:
Anguiano, B., Majewski, S. R., Allende-Prieto, C., Meszaros, S., Jönsson, H., García-Hernández, D. A., Beaton, R. L., Stringfellow, G. S., Cunha, K., Smith, V. V.
Publikováno v:
A&A 620, A76 (2018)
We undertake a critical and comprehensive comparison of the radial velocities and the main stellar atmospheric parameters for stars in common between the latest data releases from the APOGEE and the LAMOST surveys. There is a total of 42,420 dwarfs/g
Externí odkaz:
http://arxiv.org/abs/1807.07625
Autor:
Buder, S., Asplund, M., Duong, L., Kos, J., Lind, K., Ness, M. K., Sharma, S., Bland-Hawthorn, J., Casey, A. R., De Silva, G. M., D'Orazi, V., Freeman, K. C., Lewis, G. F., Lin, J., Martell, S. L., Schlesinger, K. J., Simpson, J. D., Zucker, D. B., Zwitter, T., Amarsi, A. M., Anguiano, B., Carollo, D., Cotar, K., Cottrell, P. L., Da Costa, G., Gao, X. D., Hayden, M. R., Horner, J., Ireland, M. J., Kafle, P. R., Munari, U., Nataf, D. M., Nordlander, T., Stello, Dennis, Ting, Y. -S., Traven, G., Watson, F., Wittenmyer, R. A., Wyse, R. F. G., Yong, D., Zinn, J. C., Zerjal, M.
The Galactic Archaeology with HERMES (GALAH) survey is a large-scale stellar spectroscopic survey of the Milky Way and designed to deliver chemical information complementary to a large number of stars covered by the $Gaia$ mission. We present the GAL
Externí odkaz:
http://arxiv.org/abs/1804.06041
Autor:
Duong, L., Freeman, K. C., Asplund, M., Casagrande, L., Buder, S., Lind, K., Ness, M., Bland-Hawthorn, J., De Silva, G. M., D'Orazi, V., Kos, J., Lewis, G. F., Lin, J., Martell, S. L., Schlesinger, K., Sharma, S., Simpson, J. D., Zucker, D. B., Zwitter, T., Anguiano, B., Da Costa, G. S., Hyde, E., Horner, J., Kafle, P. R., Nataf, D. M., Reid, W., Stello, D., Ting, Y. -S., Wyse, R. F. G.
Using data from the GALAH pilot survey, we determine properties of the Galactic thin and thick disks near the solar neighbourhood. The data cover a small range of Galactocentric radius ($7.9 \leq R_\mathrm{GC} \leq 9.5$ kpc), but extend up to 4 kpc i
Externí odkaz:
http://arxiv.org/abs/1801.01514
Autor:
Traven, G., Matijevič, G., Zwitter, T., Žerjal, M., Kos, J., Asplund, M., Bland-Hawthorn, J., Casey, A. R., De Silva, G., Freeman, K., Lin, J., Martell, S. L., Schlesinger, K. J., Sharma, S., Simpson, J. D., Zucker, D. B., Anguiano, B., Da Costa, G., Duong, L., Horner, J., Hyde, E. A., Kafle, P. R., Munari, U., Nataf, D., Navin, C. A., Reid, W., Ting, Y. -S.
Galah is an ongoing high-resolution spectroscopic survey with the goal of disentangling the formation history of the Milky Way, using the fossil remnants of disrupted star formation sites which are now dispersed around the Galaxy. It is targeting a r
Externí odkaz:
http://arxiv.org/abs/1612.02242
Autor:
Rebassa-Mansergas, A., Anguiano, B., García-Berro, E., Freeman, K. C., Cojocaru, R., Manser, C. J., Pala, A. F., Gänsicke, B. T., Liu, X. -W.
The age-metallicity relation (AMR) is a fundamental observational constraint for understanding how the Galactic disc formed and evolved chemically in time. However, there is not yet an agreement on the observational properties of the AMR for the sola
Externí odkaz:
http://arxiv.org/abs/1608.03064
Autor:
Anguiano, B., De Silva, G. M., Freeman, K., Da Costa, G. S., Zwitter, T., Quillen, A. C., Zucker, D. B., Navarro, J. F., Kunder, A., Siebert, A., Wyse, R. F. G., Grebel, E. K., Kordopatis, G., Gibson, B. K., Seabroke, G., Sharma, S., Wojno, J., Bland-Hawthorn, J., Parker, Q. A., Steinmetz, M., Boeche, C., Gilmore, G., Bienayme, O., Reid, W., Watson, F.
We report the identification of extended tidal debris potentially associated with the globular cluster NGC 3201, using the RAVE catalogue. We find the debris stars are located at a distance range of 1-7 kpc based on the forthcoming RAVE distance esti
Externí odkaz:
http://arxiv.org/abs/1601.02282
Autor:
Anguiano, B., Zucker, D. B., Scholz, R. -D., Grebel, E. K., Seabroke, G., Kunder, A., Binney, J., McMillan, P. J., Zwitter, T., Wyse, R. F. G., Kordopatis, G., Bienaymé, O., Bland-Hawthorn, J., Boeche, C., Freeman, K. C., Gibson, B. K., Gilmore, G., Munari, U., Navarro, J., Parker, Q., Reid, W., Siebert, A., Siviero, A., Steinmetz, M., Watson, F.
We present the identification of potential members of nearby Galactic globular clusters using radial velocities from the RAdial Velocity Experiment Data Release 4 (RAVE-DR4) survey database. Our identifications are based on three globular clusters --
Externí odkaz:
http://arxiv.org/abs/1504.07695
Autor:
De Silva, G. M., Freeman, K. C., Bland-Hawthorn, J., Martell, S., de Boer, E. Wylie, Asplund, M., Keller, S., Sharma, S., Zucker, D. B., Zwitter, T., Anguiano, B., Bacigalupo, C., Bayliss, D., Beavis, M. A., Bergemann, M., Campbell, S., Cannon, R., Carollo, D., Casagrande, L., Casey, A. R., Da Costa, G., D'Orazi, V., Dotter, A., Duong, L., Heger, A., Ireland, M. J., Kafle, P. R., Kos, J., Lattanzio, J., Lewis, G. F., Lin, J., Lind, K., Munari, U., Nataf, D. M., O'Toole, S., Parker, Q. A., Reid, W., Schlesinger, K. J., Sheinis, A., Simpson, J. D., Stello, D., Ting, Y-S., Traven, G., Watson, F., Wittenmyer, R., Yong, D., Zerjal, M.
The GALAH survey is a large high-resolution spectroscopic survey using the newly commissioned HERMES spectrograph on the Anglo-Australian Telescope. The HERMES spectrograph provides high-resolution (R ~28,000) spectra in four passbands for 392 stars
Externí odkaz:
http://arxiv.org/abs/1502.04767