Abstract
AbstractD15 Dust and gas in the inner accretion disk around the Herbig star MWC 147 resolved with infrared spectro‐interferometryD21 The effective temperature of OGLE‐TR‐10 – The Balmer α lineD29 Metal Injection into the Intracluster MediumD30 Eigenmodes of circumstellar dust shellsD40 Numerical Modelling Approach of Circumstellar Dust Shells Around Pulsating AGB Stars Aiming at Multi Time Scale ProcessesD45 UV radiation induced CO molecule formation patterns in low density PDRsD46 IR properties of calcite and dolomite at low temperaturesD47 Observations and Models of Dusty Giants – Past and PresentD51 A multi‐method approach to the outer layers of AGB starsD53 On the convective energy transport in M‐type brown dwarf atmospheresD70 Structure and Dust Composition of the TW Hya DiscD75 Chemical Abundances in the Carina Dwarf Spheroidal GalaxyD76 Kinematic and chemical constraints on the formation of M31's inner halo structuresD77 IR band profiles of silicate and oxide dust obtained by laboratory measurements of free‐flying particlesD98 Dust particle growth in protoplanetary disksD134 Comparative study of dust cloud modelling for substellar atmospheresD137 Photometric study of neglected binary DV PscD154 Quantitative Spectroscopy of DenebD160 Hot subluminous Ostars from the SDSSD166 Simultaneous Observations of Solar Ca II H and Ca II 8662 lines and Numerical Simulation of these linesD182 Present‐day carbon abundances in the solar vicinityD189 Detection of a giant planet around a pulsating extreme horizontal branch star: the oldest known planet?D200 Confirmation of a very young binary brown dwarf candidate with disk in ChamaeleonD208 Galaxy ages and metallicities in the cluster A1314D217 Charge‐dipole induced dust gelation – fastening the process of dust growth in protoplanetary disksD246 Protoplanetary Disk Structure and Evolution
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.