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19942024
most citedA diversity of dusty AGN tori: Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies

256 citations · 4.4k across the 147 of their papers we have counts for

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Showing 2013Show all

5 papers · 1 filter

astro-ph.SR2013★ 34 cited

Evidence of a discontinuous disk structure around the Herbig Ae star HD 139 614

Alexis Matter, Lucas Labadie, Alexander Kreplin +6

A new class of pre-main sequence objects has been recently identified as pre-transitional disks. They present near-infrared excess coupled to a flux deficit at about 10 microns and…

astro-ph.CO2013★ 59 cited

Evidence for a receding dust sublimation region around a supermassive black hole

Makoto Kishimoto, Sebastian F. Hoenig, Robert Antonucci +6

The near-IR emission in Type 1 AGNs is thought to be dominated by the thermal radiation from dust grains that are heated by the central engine in the UV/optical and are almost at t…

astro-ph.CO2013★ 256 cited

A diversity of dusty AGN tori: Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies

Leonard Burtscher, Klaus Meisenheimer, Konrad R. W. Tristram +9

The AGN-heated dust distribution (the "torus") is increasingly recognized not only as the absorber required in unifying models, but as a tracer for the reservoir that feeds the nuc…

astro-ph.SR2013★ 77 cited

High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER

Keiichi Ohnaka, Karl-Heinz Hofmann, Dieter Schertl +5

We present high spectral resolution aperture-synthesis imaging of the red supergiant Antares (alpha Sco) in individual CO first overtone lines with VLTI/AMBER. The reconstructed im…

astro-ph.SR2013★ 25 cited

LBT/LUCIFER near-infrared spectroscopy of PV Cephei. An outbursting young stellar object with an asymmetric jet

A. Caratti o Garatti, R. Garcia Lopez, G. Weigelt +4

We present a detailed spectroscopic investigation of the young eruptive star PV Cep, to improve our understanding of its nature and characterise its circumstellar environment after…