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20022026
most citedA Major Asymmetric Dust Trap in a Transition Disk

611 citations · 14.6k across the 256 of their papers we have counts for

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Showing 2011Show all

14 papers · 1 filter

astro-ph.GA2011★ 89 cited

Water in star-forming regions with Herschel: highly excited molecular emission from the NGC 1333 IRAS 4B outflow

Gregory J. Herczeg, Agata Karska, Simon Bruderer +9

During the embedded phase of pre-main sequence stellar evolution, a disk forms from the dense envelope while an accretion-driven outflow carves out a cavity within the envelope. Hi…

astro-ph.SR2011★ 82 cited

NUV Excess in Slowly Accreting T Tauri Stars: Limits Imposed by Chromospheric Emission

Laura Ingleby, Nuria Calvet, Edwin Bergin +20

Young stars surrounded by disks with very low mass accretion rates are likely in the final stages of inner disk evolution and therefore particularly interesting to study. We presen…

astro-ph.GA2011★ 66 cited

A 30 AU radius CO gas hole in the disk around the Herbig Ae star Oph IRS 48

Joanna M. Brown, Gregory J. Herczeg, Klaus M. Pontoppidan +1

The physical processes leading to the disappearance of disks around young stars are not well understood. A subclass of transitional disks, the so-called cold disks with large inner…

astro-ph.SR2011★ 120 cited

Modelling Herschel observations of hot molecular gas emission from embedded low-mass protostars

R. Visser, L. E. Kristensen, S. Bruderer +6

Aims. Young stars interact vigorously with their surroundings, as evident from the highly rotationally excited CO (up to Eup=4000 K) and H2O emission (up to 600 K) detected by the…

astro-ph.SR2011★ 26 cited

CO and H2 Absorption in the AA Tauri Circumstellar Disk

Kevin France, Eric B. Burgh, Gregory J. Herczeg +7

The direct study of molecular gas in inner protoplanetary disks is complicated by uncertainties in the spatial distribution of the gas, the time-variability of the source, and the…

astro-ph.GA2011★ 30 cited

Herschel observations of the Herbig-Haro objects HH52-54

P. Bjerkeli, R. Liseau, B. Nisini +11

We are aiming at the observational estimation of the relative contribution to the cooling by CO and H2O, as this provides decisive information for the understanding of the oxygen c…