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pro vyhledávání: '"Miret, F. X."'
In spite of its importance for the study of star formation at all mass domains, the nearby young sigma Orionis cluster still lacks a comprehensive survey for multiplicity. We try to fill that observational gap by looking for wide resolved binaries wi
Externí odkaz:
http://arxiv.org/abs/1707.00436
Autor:
Caballero, J. A., Genebriera, J., Tobal, T., Miret, F. X., Rica, F. M., Cairol, J., Miret, N., Novalbos, I., Montes, D., Klutsch, A.
The boundary between professional and amateur astronomers gets narrower and narrower. We present several real examples, most of them published in refereed journals, of works resulting from fruitful collaborations between key amateur astronomers in Sp
Externí odkaz:
http://arxiv.org/abs/1211.2934
LP 209-28 and LP 209-27 have similar proper motions as tabulated by several catalogues. Using seven astrometric epochs spanning 59 years, we confirm a common tangential velocity by measuring a constant angular separation of rho = 666.62+/-0.09 arcsec
Externí odkaz:
http://arxiv.org/abs/1205.5572
Autor:
Caballero, J. A., Montes, D., Klutsch, A., Genebriera, J., Miret, F. X., Tobal, T., Cairol, J., Pedraz, S.
Aims: We investigated in detail the system WDS 19312+3607, whose primary is an active M4.5Ve star previously thought to be young (tau ~ 300-500 Ma) based on high X-ray luminosity. Methods: We collected intermediate- and low-resolution optical spectra
Externí odkaz:
http://arxiv.org/abs/1006.4116
The Aladin sky atlas of the Virtual Observatory has shown to be a powerful and easy-handling tool for the discovery, confirmation, and characterisation of high proper-motion, multiple stellar systems of large separation in the solar vicinity. Some of
Externí odkaz:
http://arxiv.org/abs/0810.2030
Akademický článek
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Publikováno v:
Astronomische Nachrichten; Jan2018, Vol. 339 Issue 1, p60-71, 12p
Autor:
Caballero, J. A., Montes Gutiérrez, David, Klutsch, A., Genebriera, J., Miret, F. X., Tobal, T., Cairol, J., Pedraz, S.
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Aims. We investigated in detail the system WDS 19312+3607, whose primary is an active M4.5Ve star previously inferred to be young (τ ~ 300–500 Ma) based on its high X-ray luminosity. Methods. We collected intermediate- and low-resolution optical s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::248fe0edf26ffaf8e197138aa005cf4b
https://eprints.ucm.es/id/eprint/37822/1/davidmontes15libre.pdf
https://eprints.ucm.es/id/eprint/37822/1/davidmontes15libre.pdf
Akademický článek
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Publikováno v:
Highlights of Spanish Astrophysics V; 2010, p379-379, 1p