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20052009
most citedNon-LTE Monte Carlo Radiative Transfer: II. Non-Isothermal Solutions for Viscous Keplerian Disks

87 citations · 230 across the 6 of their papers we have counts for

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astro-ph.SR2009★ 20 cited

Toward Understanding The B[e] Phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429

A. S. Miroshnichenko, E. L. Chentsov, V. G. Klochkova +19

FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emission-line spectra and infrared excesses, which are most likely due to recently f…