Zobrazeno 1 - 10
of 22
pro vyhledávání: '"G. M. Kennedy"'
Autor:
Jonathan P Marshall, J Milli, E Choquet, C del Burgo, G M Kennedy, F Kemper, M C Wyatt, Q Kral, R Soummer
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:5940-5951
Planetesimals -- asteroids and comets -- are the building blocks of planets in protoplanetary discs and the source of dust, ice and gas in debris discs. Along with planets they comprise the left-over material after star formation that constitutes a p
Autor:
J B Lovell, M C Wyatt, P Kalas, G M Kennedy, S Marino, A Bonsor, Z Penoyre, B J Fulton, N Pawellek
$\kappa$CrB is a ${\sim}2.5\,$Gyr old K1 sub-giant star, with an eccentric exo-Jupiter at ${\sim}2.8\,$au and a debris disc at tens of au. We present ALMA Band 6 ($1.3\,$mm) and HST scattered light ($0.6\,\mu$m) images, demonstrating $\kappa$CrB's br
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acb96c033b073016cca084bc61edd120
http://arxiv.org/abs/2209.12910
http://arxiv.org/abs/2209.12910
The optical properties of the second generation dust that we observe in debris disks remain quite elusive, whether it is the absorption efficiencies at millimeter wavelengths or the (un)polarized phase function at near-infrared wavelengths. Thankfull
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3281aadedba62af5cdc08f3569823617
http://wrap.warwick.ac.uk/167251/7/WRAP-halo-around-HD-32297-um-sized-cometary-dust-2022.pdf
http://wrap.warwick.ac.uk/167251/7/WRAP-halo-around-HD-32297-um-sized-cometary-dust-2022.pdf
Autor:
M. A. Kenworthy, D. González Picos, E. Elizondo, R. G. Martin, D. M. van Dam, J. E. Rodriguez, G. M. Kennedy, C. Ginski, M. Mugrauer, N. Vogt, C. Adam, R. J. Oelkers
Publikováno v:
Astronomy & Astrophysics, 666, A61
Context. Young multiple stellar systems can host both circumstellar and circumbinary discs composed of gas and dust, and the orientations of circumbinary discs can be sculpted by the orientation and eccentricity of the central binaries. Studying mult
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::783c2ebf93c19fa8fb89d90c14b29c0d
https://doi.org/10.1051/0004-6361/202243441
https://doi.org/10.1051/0004-6361/202243441
Autor:
G. Cugno, T. D. Pearce, R. Launhardt, M. J. Bonse, J. Ma, T. Henning, A. Quirrenbach, D. Ségransan, E. C. Matthews, S. P. Quanz, G. M. Kennedy, A. Müller, S. Reffert, E. L. Rickman
Publikováno v:
Astronomy & Astrophysics, 669
Context. Planet formation is a frequent process, but little observational constraints exist about the mechanisms involved, especially for giant planets at large separation. The NaCo-ISPY large program is a 120 night L ²-band direct imaging survey ai
Publikováno v:
Astronomy & Astrophysics
Autor:
M. C. Wyatt, G. M. Kennedy
This paper considers the evidence that debris disks are self-stirred by the formation of Plutos. A model for the dust produced during self-stirring is applied to statistics for A stars. As there is no significant difference between excesses of A-star
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::171ea827d30821e0508736db8f19a52a
http://arxiv.org/abs/1002.3469
http://arxiv.org/abs/1002.3469
Publikováno v:
The American surgeon. 67(8)
Paraduodenal hernias are uncommon congenital herniations into the mesentery of the colon that present as small bowel obstruction. The diagnosis is elusive but may be made by CT scan or upper gastrointestinal series. There are three types: left, right
Publikováno v:
American journal of medical genetics. 69(3)
Charcot-Marie-Tooth (CMT) disease type 1A is an inherited peripheral neuropathy characterized by slowly progressive distal muscle wasting and weakness, decreased nerve conduction velocities, and genetic linkage to 17p12. Most (98%) CMT1A cases are ca
Autor:
D J Tolhurst, G M Kennedy
Publikováno v:
Perception. 25:85-85
Previous studies with simplified stimuli such as combinations of sinusoidal gratings have revealed phase identification losses in the periphery that are not eliminated by a scaling factor. How do these phase processing problems influence our ability