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pro vyhledávání: '"Rosales-Ortega, F. F."'
The extraplanar diffuse ionised gas is a key component for understanding the feedback processes that connect galactic discs and their halos. In this paper, we present the second study of the BETIS project, which aims to explore the ionisation mechani
Externí odkaz:
http://arxiv.org/abs/2406.17123
Autor:
González-Díaz, R., Rosales-Ortega, F. F., Galbany, L., Anderson, J. P., Jiménez-Palau, C., Kopsacheili, M., Kuncarayakti, H., Lyman, J. D., Sánchez, S. F.
Publikováno v:
A&A 687, A20 (2024)
We present the Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) project, designed for the spatial and spectral study of the diffuse ionised gas (DIG) in a selection of nearby spiral galaxies observed with the MUSE integral-field
Externí odkaz:
http://arxiv.org/abs/2311.14254
Autor:
Morales-Vargas, A., Torres-Papaqui, J. P., Rosales-Ortega, F. F., Chow-Martínez, M., Trejo-Alonso, J. J., Ortega-Minakata, R. A., Robleto-Orús, A. C., Romero-Cruz, F. J., Neri-Larios, D. M.
Galaxy evolution is generally affected by tidal interactions. Firstly, in this series, we reported several effects which suggest that tidal interactions contribute to regulating star formation (SF). To confirm that so, we now compare stellar mass ass
Externí odkaz:
http://arxiv.org/abs/2109.07731
Autor:
Morales-Vargas, A., Torres-Papaqui, J. P., Rosales-Ortega, F. F., Sánchez, S. F., Chow-Martínez, M., Ortega-Minakata, R. A., Trejo-Alonso, J. J., Robleto-Orús, A. C., Romero-Cruz, F. J., Neri-Larios, D. M.
We explore the effects of tidal interactions on star formation (SF) by analysing a sample of CALIFA survey galaxies. The sample consists of tidally and non-tidally perturbed galaxies, paired at the closest stellar mass densities for the same galaxy t
Externí odkaz:
http://arxiv.org/abs/2009.06099
Autor:
Falcón-Barroso, J., van de Ven, G., Lyubenova, M., Méndez-Abreu, J., Aguerri, J. A. L., García-Lorenzo, B., Bekeraité, S., Sánchez, S. F., Husemann, B., García-Benito, R., Delgado, R. M. González, Mast, D., Walcher, C. J., Zibetti, S., Zhu, L., Barrera-Ballesteros, J. K., Galbany, L., Sánchez-Blázquez, P., Singh, R., Bosch, R. C. E. van den, Wild, V., Bland-Hawthorn, J., Fernandes, R. Cid, de Lorenzo-Cáceres, A., Gallazzi, A., Marino, R. A., Márquez, I., Peletier, R. F., Pérez, E., Pérez, I., Roth, M. M., Rosales-Ortega, F. F., Ruiz-Lara, T., Wisotzki, L., Ziegler, B.
Publikováno v:
A&A 632, A59 (2019)
[Abridged] We present the apparent stellar angular momentum of 300 galaxies across the Hubble sequence, using integral-field spectroscopic data from the CALIFA survey. Adopting the same $\lambda_\mathrm{R}$ parameter previously used to distinguish be
Externí odkaz:
http://arxiv.org/abs/1910.06236
Publikováno v:
A&A 631, A23 (2019)
The HII regions are all studied employing the same general prescriptions, despite the possible influence of their environment in their star formation processes. Through the analysis of two samples of 725 inner and 671 outer disk HII region observed s
Externí odkaz:
http://arxiv.org/abs/1909.00465
Akademický článek
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Autor:
Fernández, Vital, Terlevich, Elena, Díaz, Angeles I., Terlevich, Roberto, Rosales-Ortega, F. F.
The primordial helium abundance $Y_P$ is calculated using sulphur as metallicity tracer in the classical methodology (with $Y_P$ as an extrapolation of $Y$ to zero metals). The calculated value, $Y_{P,\,S}=0.244\pm0.006$, is in good agreement with th
Externí odkaz:
http://arxiv.org/abs/1804.10701
Autor:
Galbany, L., Anderson, J. P., Sánchez, S. F., Kuncarayakti, H., Pedraz, S., González-Gaitán, S., Stanishev, V., Domínguez, I., Moreno-Raya, M. E., Wood-Vasey, W. M., Mourão, A. M., Ponder, K. A., Badenes, C., Mollá, M., López-Sánchez, A. R., Rosales-Ortega, F. F., Vílchez, J. M., García-Benito, R., Marino, R. A.
We present the Pmas/ppak Integral-field Supernova hosts COmpilation (PISCO) which comprises Integral Field Spectroscopy (IFS) of 232 supernova (SN) host galaxies, that hosted 272 SNe, observed over several semesters with the 3.5m telescope at the Cal
Externí odkaz:
http://arxiv.org/abs/1802.01589
Publikováno v:
A&A 609, A102 (2018)
Context. The knowledge of abundance distributions is central to understanding the formation and evolution of galaxies. Most of the relations employed for the derivation of gas abundances have so far been derived from observations of outer disk HII re
Externí odkaz:
http://arxiv.org/abs/1801.07126