RT Journal Article
T1 The Fresnel space imager as a disk evolution watcher
A1 Gómez De Castro, Ana Inés
AB The Fresnel Diffractive Imaging Arrays form high resolution images by diffraction with low radiometric efficiencies. They are extremely good devices to make high resolution imaging and integral field spectroscopy of bright sources. Thirty meter arrays will provide a spatial resolution of 0.8 mas at Lyman-alpha that will open a completely new field of research: the study of matter distribution around disks and their gravitational drives. In this contribution, the potentials of the 3.6 m precursors (or probes) for astrophysical disks and jets research, are described. Main emphasis is made on young planetary disks.
PB Springer
SN 0922-6435
YR 2011
FD 2011-06
LK https://hdl.handle.net/20.500.14352/42238
UL https://hdl.handle.net/20.500.14352/42238
LA eng
NO Gómez De Castro, A. I. «The Fresnel Space Imager as a Disk Evolution Watcher». Experimental Astronomy, vol. 30, n.o 2-3, junio de 2011, pp. 205-16. DOI.org (Crossref), https://doi.org/10.1007/s10686-011-9223-8.
NO Ministerio de Ciencia, Innovación y Universidades (España)
DS Docta Complutense
RD 7 abr 2025