Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Cervantes Sodi, Bernardo"'
Autor:
Ballesteros-Paredes, Javier, Zamora-Avilés, Manuel, Román-Zúñiga, Carlos, Palau, Aina, Cervantes-Sodi, Bernardo, Gutiérrez-Dávila, Karla, Camacho, Vianey, Jiménez-Andrade, Eric, Gazol, Adriana
We explain the large variety of star formation laws in terms of one single, simple law that can be inferred from the definition of the star formation rate and basic algebra. The resulting equation, $\SFR = \eff\ \Mcollapsing/\tauff$, although it has
Externí odkaz:
http://arxiv.org/abs/2408.13636
Autor:
Pérez-Montaño, Luis Enrique, Cervantes Sodi, Bernardo, Rodriguez-Gomez, Vicente, Zhu, Qirong, Ogiya, Go
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Sep2024, Vol. 533 Issue 1, p93-108, 16p
Autor:
Tawfeek, Amira A., Saha, Kanak, Vaghmare, Kaustubh, Kembhavi, A.K., Takey, Ali, Cervantes Sodi, Bernardo, Fritz, Jacopo, Awad, Zainab, Ali, Gamal B., Hayman, Z.M.
Publikováno v:
In New Astronomy August 2021 87
We present a study of the connection between the galactic spin parameter $\lambda_{d}$ and the bar fraction in a volume-limited sample of 10,674 disk galaxies drawn from the Sloan Digital Sky Survey Data Release 7. The galaxies in our sample are visu
Externí odkaz:
http://arxiv.org/abs/1303.3696
We study the evolution of the galactic spin using data of high redshift galaxies in the fields of the Great Observatories Origins Deep Survey (GOODS). Through simple dynamical considerations we estimate the spin for the disc galaxies in our sample an
Externí odkaz:
http://arxiv.org/abs/1204.4236
Publikováno v:
The Astrophysical Journal Letters 735 (2011), L25
Using an extensive sample of galaxies selected from the Sloan Digital Sky Survey Data Release 5, we compare the angular momentum distribution of active galactic nucleus (AGN) with non-AGN hosting late-type galaxies. To this end we characterize galact
Externí odkaz:
http://arxiv.org/abs/1103.3542
Publikováno v:
AIP Conf.Proc.1240:407-408,2010
To study if the angular momentum gain for each member of a galaxy pair was the result of tidal torques imprinted by the same tidal field, we search for correlations between the spin in pairs of spiral galaxies identified using the Sloan Digital Sky S
Externí odkaz:
http://arxiv.org/abs/0912.1151
Autor:
Zhu, Qirong, Pérez-Montaño, Luis Enrique, Rodriguez-Gomez, Vicente, Cervantes Sodi, Bernardo, Zjupa, Jolanta, Marinacci, Federico, Vogelsberger, Mark, Hernquist, Lars
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2023, Vol. 523 Issue 3, p3991-4014, 24p
The relation between morphology, star formation history, and environment in local Universe galaxies.
Autor:
Pérez-Millán, David, Fritz, Jacopo, González-Lópezlira, Rosa A, Moretti, Alessia, Cervantes Sodi, Bernardo, Vulcani, Benedetta, Gullieuszik, Marco, Bruzual, Gustavo, Charlot, Stéphane, Bettoni, Daniela
Publikováno v:
Monthly Notices of the Royal Astronomical Society; May2023, Vol. 521 Issue 1, p1292-1315, 24p
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