Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Docobo, J. A."'
Autor:
Masda, Suhail, Docobo, J. A., Hussein, A., Mardini, M., Al-Ameryeen, H., Campo, P., Khan, A., Pathan, J.
The precise determination of the physical and dynamical parameters of the HIP 109951 triple star system (WDS J22161-0705AB) which is formed by the A, Ba, and Bb components are presented. The binary nature of component B was recently confirmed by stud
Externí odkaz:
http://arxiv.org/abs/1911.09972
Autor:
Madiedo, J. M., Zamorano, J., Trigo-Rodriguez, J. M., Ortiz, J. L., Docobo, J. A., Izquierdo, J., Lacruz, J., Campo, P. P., Andrade, M., Pastor, S., Reyes, J. A. de los, Ocaña, F., de Miguel, A. Sanchez, Pujols, P.
We analyze the outburst experienced by the September $\varepsilon$-Perseid meteor shower on 9 September 2013. As a result of our monitoring the atmospheric trajectory of 60 multi-station events observed over Spain was obtained and accurate orbital da
Externí odkaz:
http://arxiv.org/abs/1807.06364
A complete astrophysical and dynamical study of the close visual binary system (CVBS) (A7V + F0V), Finsen 350, is presented. Beginning with the entire observational spectral energy distribution (SED) and the magnitude difference between the subcompon
Externí odkaz:
http://arxiv.org/abs/1802.03811
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 459, Issue 2, p.1580-1585, 2016
Improved orbits are presented for the visual binaries WDS 02366+1227, WDS 02434-6643, WDS 03244-1539, WDS 08507+1800, WDS 09128-6055, WDS 11532-1540, WDS 17375+2419, and WDS 22408-0333. The latest orbits for these binaries were demonstrating a great
Externí odkaz:
http://arxiv.org/abs/1609.03392
Publikováno v:
Astrophysics and Space Science, Volume 361, article id.105, 2016
We have selected a set of 17 visual binaries that demonstrate great inconsistency between the systemic mass obtained through Kepler's Third Law as compared to that calculated through standard mass-luminosity and mass-spectrum relationships. A careful
Externí odkaz:
http://arxiv.org/abs/1609.00487
Autor:
Monzón, C. V.1,2 (AUTHOR) carlos.vazquez.monzon@rai.usc.es, Docobo, J. A.1,2,3,4 (AUTHOR)
Publikováno v:
Astrophysics & Space Science. May2023, Vol. 368 Issue 5, p1-16. 16p.
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Autor:
Kraus, S., Weigelt, G., Balega, Y. Y., Docobo, J. A., Hofmann, K. -H., Preibisch, T., Schertl, D., Tamazian, V. S., Driebe, T., Ohnaka, K., Petrov, R., Schoeller, M., Smith, M.
The nearby high-mass star binary system Theta 1 Orionis C is the brightest and most massive of the Trapezium OB stars at the core of the Orion Nebula Cluster, and it represents a perfect laboratory to determine the fundamental parameters of young hot
Externí odkaz:
http://arxiv.org/abs/0902.0365