Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Hector Aceves"'
Autor:
Carlos E Chavez, Nikolaos Georgakarakos, Andres Aviles, Hector Aceves, Gagik Tovmassian, Sergey Zharikov, J E Perez–Leon, Francisco Tamayo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:4629-4638
Some Cataclysmic Variables (CVs) exhibits a very long photometric period (VLPP). We calculate the properties of a hypothetical third body, initially assumed on circular--planar orbit, by matching the modelled VLPP to the observed one of four CVs stud
Autor:
Sergey Zharikov, Cesar Ramos, Gagik Tovmassian, Hector Aceves, Carlos E. Chavez, Nikolaos Georgakarakos, Andres Aviles
A very long term variability (VLPP), with period of 875 days, was observed in the long-term light curve of FS Aurigae in 2011. This periodicity was calculated on 6 cycles. We re-examine the periodicity with new observations over of the past 5 yrs. A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abbd9d234eb5412262c0f2342e5826cf
http://arxiv.org/abs/2301.04286
http://arxiv.org/abs/2301.04286
Autor:
I. Arias, A. Avilés, F. J. Tamayo, J. E. Pérez, Carlos E. Chavez, Eduardo Pérez-Tijerina, Hector Aceves
Publikováno v:
Revista Mexicana de Astronomía y Astrofísica. 56:11-18
We present observational evidence that helps classify the non-eclipsing binary system SDSSJ 122405.58+184102.7 as a new member of the SW Sextantis (SW Sex) class. First, from the analysis of the optical light curve, we identify the presence of two pe
Autor:
Hector Aceves, F. G. Ramon-Fox
Galaxy interactions can have an important effect in a galaxy's evolution. Cosmological models predict a large number of small satellites around galaxies. It is important to study the effect that these small satellites can have on the host. The presen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::572674b5d37b3aff2a57518cca940d70
http://arxiv.org/abs/1901.00510
http://arxiv.org/abs/1901.00510
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, vol 474, iss 2
Krumpe, M; Miyaji, T; Coil, AL; & Aceves, H. (2018). Spatial clustering and halo occupation distribution modelling of local AGN via cross-correlation measurements with 2MASS galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 474(2), 1773-1786. doi: 10.1093/mnras/stx2705. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/32n1n73x
Monthly Notices of the Royal Astronomical Society, vol 474, iss 2
Krumpe, M; Miyaji, T; Coil, AL; & Aceves, H. (2018). Spatial clustering and halo occupation distribution modelling of local AGN via cross-correlation measurements with 2MASS galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 474(2), 1773-1786. doi: 10.1093/mnras/stx2705. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/32n1n73x
Monthly Notices of the Royal Astronomical Society, vol 474, iss 2
We present the clustering properties and halo occupation distribution (HOD) modelling of very low redshift, hard X-ray-detected active galactic nuclei (AGN) using cross-correlation function measurements with Two-Micron All Sky Survey galaxies. Spanni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b88c62b84072d49320b3f40e8aeb836
https://escholarship.org/uc/item/32n1n73x
https://escholarship.org/uc/item/32n1n73x
Publikováno v:
EPJ Web of Conferences, Vol 186, p 12008 (2018)
We analyzed the scientific production of astronomers published in the first Mexican journal of astronomy, the Boletín de losObservatorios de Tonantzintla y Tacubaya (BOTT), from 1952 to 1972. The bibliometric behavior of the BOTT is provided, identi
Autor:
M. Carmen Eliche-Moral, Trinidad Tapia, Hector Aceves, Alejandro Borlaff, Cristina Rodríguez-Pérez, Miguel Querejeta
(Abridged version) We explore whether a scenario that combines an origin by mergers at $z\sim$1.8-1.5 with a subsequent passive evolution of the resulting S0 remnants since $z \sim$0.8-1 is compatible with observational data of S0s in the Tully-Fishe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af677be834cca17b115dd51c98f94dea
http://arxiv.org/abs/1706.03803
http://arxiv.org/abs/1706.03803
Publikováno v:
Astrophysical Journal, vol 815, iss 1
Krumpe, M; Miyaji, T; Husemann, B; Fanidakis, N; Coil, AL; & Aceves, H. (2015). THE SPATIAL CLUSTERING of ROSAT ALL-SKY SURVEY ACTIVE GALACTIC NUCLEI. IV. MORE MASSIVE BLACK HOLES RESIDE in MORE MASSIVE DARK MATTER HALOS. Astrophysical Journal, 815(1). doi: 10.1088/0004-637X/815/1/21. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/9vn858p4
The Astrophysical Journal, vol 815, iss 1
Krumpe, M; Miyaji, T; Husemann, B; Fanidakis, N; Coil, AL; & Aceves, H. (2015). THE SPATIAL CLUSTERING of ROSAT ALL-SKY SURVEY ACTIVE GALACTIC NUCLEI. IV. MORE MASSIVE BLACK HOLES RESIDE in MORE MASSIVE DARK MATTER HALOS. Astrophysical Journal, 815(1). doi: 10.1088/0004-637X/815/1/21. UC San Diego: Retrieved from: http://www.escholarship.org/uc/item/9vn858p4
The Astrophysical Journal, vol 815, iss 1
This is the fourth paper in a series that reports on our investigation of the clustering properties of active galactic nuclei (AGN) identified in the ROSAT All-Sky Survey (RASS) and Sloan Digital Sky Survey (SDSS). In this paper we investigate the ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::731e8eb2fe20aa973a66d1e447459d5a
https://escholarship.org/uc/item/9vn858p4
https://escholarship.org/uc/item/9vn858p4
Autor:
Hector Aceves, Maria Colosimo
Publikováno v:
American Journal of Physics. 75:139-147
An introductory exposition of Chandrasekhar’s gravitational dynamical friction, appropriate for an undergraduate class in mechanics, is presented. This friction results when a heavy particle moving through a “sea” of much lighter star particles
Autor:
Héctor Velázquez, Hector Aceves
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 360:L50-L54
We set up a series of self-consistent N-body simulations to investigate the fundamental plane of merger remnants of spiral galaxies. These last ones are obtained from a theoretical Tully-Fisher relation at z=1, assuming a constant mass-to-light ratio