Search Results - "GOMEZ DE CASTRO, Ana I"
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Photoelectric Charging of Dust Grains in the Environment of Young Stellar Objects
Published in The Astrophysical journal (20-10-2011)“…The evolution of disks around young stellar objects (YSOs) is deeply affected by the YSOs' ultraviolet (UV) radiation field especially in the 500-1100 A…”
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Variation of the ultraviolet extinction law across the Taurus-Auriga star-forming complex. A GALEX based study
Published in Monthly notices of the Royal Astronomical Society (01-06-2015)“…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…”
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3
WSO-UV progress and expectations
Published in Astrophysics and space science (01-11-2014)“…The World Space Observatory Ultraviolet (WSO-UV) is the space mission that will grant access to the ultraviolet (UV) range in the post Hubble epoch. WSO-UV is…”
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4
Polarized microwave emission from space particles in the upper atmosphere of the Earth
Published in Monthly notices of the Royal Astronomical Society (10-10-2023)“…ABSTRACT Tons of space particles enter the Earth atmosphere every year, being detected when they produce fireballs, meteor showers, or when they impact the…”
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AK Sco, First Detection of a Highly Disturbed Atmosphere in a Pre-Main-Sequence Close Binary
Published in The Astrophysical journal (20-06-2009)Get full text
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Accretion and Intercycle Variations in the PMS Interacting Binary AK Sco
Published in The Astrophysical journal (01-12-2020)“…There are only a handful of known short-period pre-main-sequence spectroscopic binaries with significant accretion rates (Class II sources). AK Sco stands out…”
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Formation of Dust Filaments in the Diffuse Envelopes of Molecular Clouds
Published in The Astrophysical journal (01-02-2021)“…The path to understanding star formation processes begins with the study of the formation of molecular clouds. The outskirts of these clouds are characterized…”
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Building galaxies, stars, planets and the ingredients for life between the stars. The science behind the European Ultraviolet-Visible Observatory
Published in Astrophysics and space science (01-11-2014)“…This contribution gathers the contents of the white paper submitted by the UV community to the Call issued by the European Space Agency in March 2013, for the…”
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Evidence of Stellar-driven Outflows from the Classical T Tauri Star RY Tau
Published in The Astrophysical journal (01-01-2007)Get full text
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The formation of planetary disks and winds: an ultraviolet view
Published in Astrophysics and space science (01-04-2009)“…Planetary systems are angular momentum reservoirs generated during star formation. This accretion process produces very powerful engines able to drive the…”
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11
Pre main sequence stars as UV sources for the World Space Observatory-UV mission
Published in Astrophysics and space science (01-09-2011)“…Pre-main sequence stars are bright UV (UV) sources compared with their main sequence analogues. The source of this excess is the high energy processes…”
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EXTENDED MAGNETOSPHERES IN PRE-MAIN-SEQUENCE EVOLUTION: FROM T TAURI STARS TO THE BROWN DWARF LIMIT
Published in The Astrophysical journal (20-04-2012)“…Low-mass pre-main-sequence stars, i.e., T Tauri stars (TTSs), strongly radiate at high energies, from X-rays to the ultraviolet (UV). This excess radiation…”
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Evidence of accretion triggered oscillations in the pre-main-sequence interacting binary AK Sco
Published in Monthly notices of the Royal Astronomical Society. Letters (11-02-2013)“…Pre-main sequence (PMS) binaries are surrounded by circumbinary discs from which matter falls on to both components. The material dragged from the circumbinary…”
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Imaging and Characterization of Extrasolar Planets with the Next Generation of Space Telescopes
Published in Geosciences (Basel) (01-12-2018)“…The study and characterization of the exoplanets’ atmospheres and composition is in its infancy. The large facilities that will make feasible to image an…”
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On the source of dense outflows from T Tauri stars — II. Warm disc winds
Published in Monthly notices of the Royal Astronomical Society (11-09-2005)“…Recent ultraviolet (UV) observations suggest that there is a hot (Te≃ 80 000 K) and dense (Ne ≃ 1010 cm−3) wind associated with the large-scale jets observed…”
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The Imaging and Slitless Spectroscopy Instrument for Surveys (ISSIS): expected radiometric performance, operation modes and data handling
Published in Astrophysics and space science (01-11-2014)“…ISSIS is the instrument for imaging and slitless spectroscopy on-board WSO-UV. In this article, a detailed comparison between ISSIS expected radiometric…”
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World Space Observatory-Ultraviolet: ISSIS, the imaging instrument
Published in Advances in space research (15-03-2014)“…The Imaging and Slitless Spectroscopy Instrument (ISSIS) will be flown as part of the science instrumentation in the World Space Observatory-Ultraviolet…”
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Challenges on Ultraviolet Astronomy 2014
Published in Astrophysics and space science (01-11-2014)“…Issue Title: Challenges on Ultraviolet Astronomy 2014…”
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Graphite to diamond transition induced by photoelectric absorption of ultraviolet photons
Published in Scientific reports (28-01-2021)“…The phase transition from graphite to diamond is an appealing object of study because of many fundamental and also, practical reasons. The out-of-plane…”
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UV Monochromatic Imaging of the Protoplanetary Nebula Hen 3-1475 Using HST STIS
Published in Galaxies (14-12-2018)“…Collimated outflows and jets play a critical role in shaping planetary nebulae (PNe), especially in the brief transition from a spherical AGB envelope to an…”
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