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19972008
most citedA quasi-time-dependent radiative transfer model of OH104.9+2.4

9 citations · 18 across the 3 of their papers we have counts for

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astro-ph20081 cited

Dissecting Massive YSOs with Mid-Infrared Interferometry

H. Linz, Th. Henning, B. Stecklum +4

The very inner structure of massive YSOs is difficult to trace. With conventional observational methods we often identify structures still several hundreds of AU in size. But we al…

astro-ph20059 cited

A quasi-time-dependent radiative transfer model of OH104.9+2.4

D. Riechers, Y. Balega, T. Driebe +4

We investigate the pulsation-phase dependent properties of the circumstellar dust shell (CDS) of the OH/IR star OH104.9+2.4 based on radiative transfer modeling (RTM) using the cod…

astro-ph20048 cited

High-resolution near-infrared speckle interferometry and radiative transfer modeling of the OH/IR star OH 104.9+2.4

D. Riechers, Y. Balega, T. Driebe +3

We present near-infrared speckle interferometry of the OH/IR star OH 104.9+2.4 in the K' band obtained with the 6m telescope of the Special Astrophysical Observatory (SAO). At a wa…

astro-ph2000

The ISO-LWS map of the Serpens cloud core: I. The SEDs of the IR/SMM sources

B. Larsson, R. Liseau, A. B. Men'shchikov +11

ISO-LWS mapping observations of the Serpens molecular cloud core are presented. The spectral range is 50 - 200 micron and the map size is 8' X 8'. These observations suffer from se…

astro-ph2000

The dynamical evolution of the fragmented, bipolar dust shell around the carbon star IRC +10216: Rapid changes of a PPN-like structure?

R. Osterbart, Y. Balega, T. Bloecker +2

We present high-resolution J-, H-, and K-band observations and the first H-K color image of the carbon star IRC +10216. The images were reconstructed from 6m telescope speckle inte…

astro-ph2000

The dynamical evolution of the dust shell of IRC+10216

R. Osterbart, Y. Balega, T. Bloecker +2

We present high-resolution J-, H-, and K-band observations of the carbon star IRC+10216. The images were reconstructed from 6 m telescope speckle interferograms using the bispectru…