Showing 1–20 of 24 results
/ Date/ Name
Feb 20, 2019Luminosity outburst chemistry in protoplanetary discs: going beyond standard tracersApr 10, 2019Revealing dust segregation in protoplanetary discs with the help of multi-frequency spectral index mapsOct 9, 2017Gas mass tracers in protoplanetary disks: CO is still the bestMar 10, 2021Gravitoviscous protoplanetary disks with a dust component. V. The dynamic model for freeze-out and sublimation of volatilesSep 6, 2018Chemical Signatures of the FU Ori OutburstsJan 13, 2018Global photometric analysis of galactic HII regionsFeb 13, 2026Tracking the dynamical, chemical and spectral evolution of molecular cores with PrestaLine: GorynychFeb 12, 2020Chemical modelling of FU Ori protoplanetary disksOct 5, 2006Anisotropy of Magnetohydrodynamic Turbulence and Polarization of the Spectral Lines of MoleculesSep 28, 2007Do we need to know the temperature in prestellar cores?Aug 17, 2023Analysis of the interstellar matter at the periphery of the supershell surrounding the CYG OB1 association in 2.12 micron molecular hydrogen lineFeb 5, 2011Polycyclic aromatic hydrocarbons in the dwarf galaxy IC 10Mar 22, 2006CB17: Inferring the dynamical history of a prestellar core with chemo-dynamical modelsJul 2, 2006Gas-phase CO in protoplanetary disks: a challenge for turbulent mixingApr 23, 2001Spectra of Maser Radiation from a Turbulent, Circumnuclear Accretion Disk. III. Circular polarizationDec 4, 2002Reduction of chemical networks. I. The case of molecular cloudsNov 19, 2003On the Influence of Uncertainties in Chemical Reaction Rates on Results of the Astrochemical ModellingJul 23, 2004Irregular Magnetic Fields and the Far-Infrared Polarimetry of Dust Emission from Interstellar CloudsJul 30, 2001Theory and Extragalactic MasersMar 23, 2004Reduction of chemical networks. II. Analysis of the fractional ionisation in protoplanetary discs