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20082026
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 7.8k across the 138 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.GA2011★ 45 cited

Herschel Observations of the T Cha Transition Disk: Constraining the Outer Disk Properties

Lucas A. Cieza, Johan Olofsson, Paul M. Harvey +7

T Cha is a nearby (d = 100 pc) transition disk known to have an optically thin gap separating optically thick inner and outer disk components. Huelamo et al. (2011) recently report…

astro-ph.EP2011★ 87 cited

Hot exozodiacal dust resolved around Vega with IOTA/IONIC

D. Defrère, O. Absil, J. -C. Augereau +10

Although debris discs have been detected around a significant number of main-sequence stars, only a few of them are known to harbour hot dust in their inner part where terrestrial…

astro-ph.SR2011★ 11 cited

Ruling out unresolved binaries in five transitional disks VLT/NACO: deep 2.12 and 1.75 μm narrow-band imaging

Silvia Vicente, Bruno Merın, Markus Hartung +8

Aims. We aim at detecting the presence of companions inside the inner hole/gap region of a sample of five well known transitional disks using spatially-resolved imaging in the near…

astro-ph.SR2011★ 48 cited

Low abundance, strong features: Window-dressing crystalline forsterite in the disk wall of HD 100546

G. D. Mulders, L. B. F. M. Waters, C. Dominik +10

Forsterite is one of the crystalline dust species that is often observed in protoplanetary disks and solar system comets. Being absent in the interstellar medium, it must be produc…

astro-ph.EP2011★ 63 cited

On the Evolution of Dust Mineralogy, From Protoplanetary Disks to Planetary Systems

Isa Oliveira, Johan Olofsson, Klaus M. Pontoppidan +3

Mineralogical studies of silicate features emitted by dust grains in protoplanetary disks and Solar System bodies can shed light on the progress of planet formation. The significan…

astro-ph.SR2011★ 42 cited

Warm dust resolved in the cold disk around T Cha with VLTI/AMBER

J. Olofsson, M. Benisty, J. -C. Augereau +12

The transition between massive Class II circumstellar disks and Class III debris disks, with dust residuals, has not yet been clearly understood. Disks are expected to dissipate wi…