Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Fatima Lopez-Martinez"'
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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There is a growing interest in the automated characterization of open clusters using data from the Gaia mission. This work evidences the importance of choosing an appropriate sampling radius (the radius of the circular region around the cluster used
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 448:484-501
The atmospheric structure of T Tauri Stars (TTSs) and its connection with the large scale outflow is poorly known. Neither the effect of the magnetically mediated inter- action between the star and the disc in the stellar atmosphere is well understoo
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
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E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
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E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The C II] feature at ~2325 Angstrom is very prominent in the spectra of T Tauri stars (TTSs). This feature is a quintuplet of semiforbidden transitions excited at electron temperatures around 10,000 K that, together with the nearby Si II] and Fe II]
Autor:
Juan A. Larruquert, Ana I. Gómez de Castro, Pablo Rodríguez, M. Gomez, Fatima Lopez-Martinez, Tomás Belenguer, Jesús Maíz, Paola Sestito, José A. Méndez, Víctor Rodrigo-Gudiel
Publikováno v:
Astrophysics and Space Science. 335:283-289
ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (
Autor:
Ana I. Gómez de Castro, Javier Lopez-Santiago, Néstor Sánchez, Fatima Lopez-Martinez, Elisa de Castro, M. Cornide
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Taurus-Auriga molecular complex (TMC) is the main laboratory for the study of low mass star formation. The density and properties of interstellar dust are expected to vary across the TMC. These variations trace important processes such as dust nu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f8a54dae989569637ad015011cc843fd
https://eprints.ucm.es/id/eprint/31322/1/1503.02404v1.pdf
https://eprints.ucm.es/id/eprint/31322/1/1503.02404v1.pdf
Autor:
Néstor Sánchez, Javier López-Santiago, Ana I. Gómez de Castro, M. Cornide, Fatima Lopez-Martinez, Javier Yañez Gestoso, P. Sestito, Elisa de Castro
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
In this work, we identify 63 bona fide new candidates to T Tauri stars (TTSs) in the Taurus-Auriga region using as baseline its ultraviolet excess. The initial data set has been defined from the GALEX all sky survey (AIS). The GALEX satellite obtaine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abc98a85a018e2c49febf432da17db8d
http://arxiv.org/abs/1412.3002
http://arxiv.org/abs/1412.3002
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
We analyze 359 ultraviolet tiles from the All Sky Imaging Survey of the space mission GALEX covering roughly 400 square degrees toward the Orion star-forming region. There is a total of 1,555,174 ultraviolet sources that were cross-matched with other
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e72eb7297ac9443acc1f23f08e4ab53
Autor:
M. Gomez, José M. Quintana, Marcos Ubierna, Jacinto Muñoz, Ana I. Gómez de Castro, Paola Sestito, Fatima Lopez-Martinez, Juan Seijas, Néstor Sánchez, Pablo Rodríguez
Publikováno v:
Advances in Space Research, ISSN 0273-1177, 2014-03, Vol. 53, No. 6
Archivo Digital UPM
Universidad Politécnica de Madrid
Archivo Digital UPM
Universidad Politécnica de Madrid
The Imaging and Slitless Spectroscopy Instrument (ISSIS) will be flown as part of the Science Instrumentation in the World Space Observatory-Ultraviolet (WSO-UV). ISSIS will be the first UV imager to operate in a high Earth orbit from a 2-m class spa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d072c5a24e75308d926ce5280047a827
Autor:
Marcos Ubierna, Néstor Sánchez, José M. Quintana, Jacinto Muñoz, Paola Sestito, Ana I. Gómez de Castro, Fatima Lopez-Martinez, Pablo Rodríguez, Juan Seijas, M. Gomez
Publikováno v:
SPIE Proceedings.
ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory - Ultraviolet (WSO-UV), a 170 cm space telescope to be launched in late 2015. ISSIS is a multipurpose instrument designed to carry out high resolution and high