activity
20032009
most citedProperties of gravitoturbulent accretion disks

144 citations · 246 across the 7 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2009144 cited

Properties of gravitoturbulent accretion disks

Roman R. Rafikov

We explore the properties of cold gravitoturbulent accretion disks - non-fragmenting disks hovering on the verge of gravitational instability - using a realistic prescription for t…

astro-ph200852 cited

Stellar proper motion and the timing of planetary transits

Roman R. Rafikov

Duration and period of transits in extrasolar planetary systems can exhibit long-term variations for a variety of reasons. Here we investigate how systemic proper motion, which ste…

astro-ph20073 cited

Stellar growth by disk accretion: the effect of disk irradiation on the protostellar evolution

Roman R. Rafikov

Young stars are expected to gain most of their mass by accretion from a disk that forms around them as a result of angular momentum conservation in the collapsing protostellar clou…

astro-ph20072 cited

Cooling of young stars growing by disk accretion

Roman Rafikov

In the initial formation stages young stars must acquire a significant fraction of their mass by accretion from a circumstellar disk that forms in the center of a collapsing protos…

astro-ph200624 cited

Microwave emission from spinning dust in circumstellar disks

Roman R. Rafikov

In the high density environments of circumstellar disks dust grains are expected to grow to large sizes by coagulation. Somewhat unexpectedly, recent near-IR observations of PAH fe…

astro-ph200621 cited

Structure of Passive Circumstellar Disks: Beyond the Two-Temperature Approximation

Roman R. Rafikov, Fabio De Colle

Structure and spectral energy distributions (SEDs) of externally irradiated circumstellar disks are often computed on the basis of the two-temperature model of Chiang & Goldreich.…