M1-92 revisited: the chemistry of an ejected common envelope Alcolea Javier Observatorio Astronómico Nacional The detailed chemical abundance pattern of the metal-rich Galactic globular cluster NGC 6366 Alves-Brito Alan Federal University of Rio Grande do Sul Carbon Enrichment in the Early Universe Andersen Johannes University of Copenhagen RAMSES II - Raman Search for Extragalactic Symbiotic Stars Angeloni Rodolfo Universidad de La Serena Observational Properties of Miras in the KELT Survey Arnold Robert Lehigh University A THEORY AND SIMULATION-BASED CONVECTIVE BOUNDARY MIXING MODEL FOR AGB STAR EVOLUTION AND Battino Umberto University of Edinburgh ElementalNUCLEOSYNTHESIS abundances of primary stars in Sirius-like systems: Constraints on pollution from AGB stars Bharat Kumar Yerra National Astronomical Observatories, Chinese Academy of Sciences On the nature and mass loss of Bulge OH/IR stars Blommaert Joris Astronomy and Astrophysics Research Group, Vrije Universiteit Jet formation revealed in post-AGB binaries Bollen Dylan MacquarieBrussel University Where is the metallicity ceiling to form carbon stars? Boyer Martha STScI To Be or Not to Be: EHB Stars and AGB Stars Brown David Specola Vaticana The discovery of an asymmetric detached shell around the "fresh" carbon AGB star TX Psc Brunner Magdalena Institut für Astrophysik Imaging Red Supergiants with VLT/SPHERE/ZIMPOL Cannon Emily KU Leuven The Impact of Dust/Gas Ratios on Chromospheric Activity in Red Giant and Supergiant Stars Carpenter Ken NASA's GSFC Metallic Line Doubling in the Spectra of the Variable R Scuti Star chafouai khadija Cadi Ayyad Raman and Thomson Wings around Balmer Lines in the Two S-Type Symbiotic Stars Z Andromedae and AG Draconis Chang Seok-Jun Department of Physics and Astronomy, Sejong University Populations of accreting white dwarfs Chen Hai-Liang Yunnan Observatories Preparing spectrophotometric and interferometric observables from 3D hydrodynamical simulations of AGB stars. Chiavassa Andrea Observatoire de la Cote d'Azur New PARSEC-V2.0 stellar isochrones with alpha-enhanced mixtures and rotation Costa Guglielmo SISSA The Role of Shocks in the Detemination of Empirical Abundances for Type-I Planetary Nebulae Costa Roberto Universidade de São Paulo Unravelling the sulphur chemistry of AGB stars Danilovich Taïssa KU Leuven APEX spectral scan of the M-type AGB star R Dor De Beck Elvire Chalmers University of Technology In search of the fundamentals of dust formation around evolved stars with the Origins Space Telescope De Beck Elvire Chalmers University of Technology Magritte: a new multidimensional accelerated general-purpose radiative transfer code De Ceuster Frederik KU Leuven Alien visitors rule cosmic makeup Decin Leen Institute of Astronomy, KU Leuven Gaseous metal oxides and hydroxides tracing the formation of AGB dust grains. Decin Leen Institute of Astronomy, KU Leuven Stacking analysis of the HERITAGE data to statistically study far-IR dust emission from evolved stars Dharmawardena Thavisha Academia Sinica Institute of Astronomy and Astrophysics Stark broadening data for post AGB and AGB stars - STARK-B Database, a node of Virtual Atomic and Molecular Data Center (VAMDC) Dimitrijevic Milan S. Astronomical Observatory Observations of the Ultraviolet-Bright Star Barnard 29 in the Globular Cluster M13 (NGC 6205) Dixon William Space Telescope Science Institute A systematic survey of grain growth in discs around post-AGB binaries with PACS and SPIRE photometry Dsilva Karan KU Leuven, Belgium A new Python interface for the spectroscopic data analysis. El jariri Youssef Cadi Aayad University The loss of large amplitude pulsations at the end of AGB evolution Engels Dieter Hamburger Sternwarte Photometric properties for a carbon star DARWIN model grid Eriksson Kjell Uppsala university Using barium stars to constrain binary interaction in systems containing stars with convective envelopes Escorza Ana Institute of Astronomy (KU Leuven) Ammonia in carbon rich stars Etmanski Bartosz Nicolaus Copernicus Astronomical Centre Grid of realistic CSPNs atmosphere models Fierro-Santillán Celia Instituto Politécnico Nacional The maser emitting structure and time variability of the SiS lines J=14-13 and 15-14 in IRC+10216 Fonfria Jose Pablo Instituto de Fisica Fundamental, CSIC Central Stars of Planetary Nebulae in Galactic Open Clusters: Providing additional data for the White Dwarf Initial-to-Final-Mass Relation Fragkou Vasiliki The University of Hong Kong On cylindrically symmetric solutions of polarized radiative transfer equation Freimanis Juris Ventspils University College Hen 3-160 - the first symbiotic binary with Mira variable S star? Galan Cezary Nicolaus Copernicus Astronomical Center PAS GK Car and GZ Nor: Two depleted low-luminosity Galactic RV Tauri stars Gezer Ilknur Ege University Infrared light curves of dusty & metal-poor AGB stars Goldman Steve Space Telescope Science Institute Mid-IR spectroscopic observations of the dustiest AGB stars in the Galaxy Goldman Steve Space Telescope Science Institute A step further on the physical, kinematic and excitation properties of PNe Gonçalves Denise R. Valongo Observatory - Federal University of Rio e Janeiro Tracers of stellar mass loss: Mid-IR colors and surface brightness fluctuations Gonzalez-Lopezlira Rosa Amelia IRyA, UNAM Using Blue Straggler Binaries to Constrain AGB Mass Transfer Gosnell Natalie Colorado College The longest period Long Period Variables in the Magellanic Clouds Groenewegen Martin Koninklijke Sterrenwacht van Belgie Differentially rotating white dwarfs with 2DStars Halabi Ghina Institute of Astronomy Heavy puzzle pieces: Learning about the i process from Pb abundances Hampel Melanie Monash Centre for Astrophysics Kepler K2: A Search for Very Red Stellar Objects Hartig Erich University of Vienna, Astrophysics Galactic Simulations of r-process Elemental Abundances Haynes Chris University of Hertfordshire Raman-Scattered O VI 6825, 7082Å and C II 7023, 7053Å in the Symbiotic Nova RR Telescopii Heo Jeong-Eun Sejong University The Structure of the Inner Circumstellar Shell in Miras Hinkle Kenneth NOAO Multiband study of AGB stars in clusters Hojaev Alisher S. UB Astronomical Institute of UAS Rotating disks around M-type AGB stars homan ward KU Leuven Variability in Post-AGB Stars: Pulsation and Binarity in Proto-Planetary Nebulae Hrivnak Bruce Valparaiso University On the silicate crystallinities of oxygen-rich evolved stars and their mass-loss rates Jiang Biwei Department of Astronomy, Beijing Normal University Binary evolution and double sequences of blue stragglers in globular clusters Jiang Dengkai Yunnan Observatories, Chinese Academy of Sciences Dust producing AGB stars in the Metal-poor, Dwarf Irregular Galaxies Sextans A and Leo A Jones Olivia UK Astronomy Technology Center Spectroscopic binaries among AGB stars Jorissen Alain ULB - Institut d'Astronomie ALMA spectrum of the extreme OH/IR star OH26.5+0.6 Justtanont Kay Chalmers University of Technology When binaries keep track of recent AGB nucleosynthesis: The Zr - Nb pair in extrinsic stars as an efficient s-process diagnostic Karinkuzhi Drisya Bangalore University The mineralogy of AGB dust in the Magellanic Clouds Kemper Ciska Academia Sinica, Institute of Astronomy & Astrophysics Monitoring of the AGB star R Doradus using SPHERE/ZIMPOL Khouri Theo Chalmers University of Technology Tomography of the red supergiant star mu Cep Kravchenko Kateryna Institute of Astronomy and Astrophysics, Universite Libre de Chemical enrichment of galaxies as the result of organic synthesis in evolved stars Kwok Sun UniversityBruxelles of British Columbia O-rich LPVs in the X-shooter Spectral Library Lançon Ariane Observatoire astronomique de Strasbourg Late Thermal Pulse Evolution Models and the Rapid Evolution of V839 Ara Lawlor Timothy Pennsylvania State University - Brandywine Carbon and oxygen isotopes in AGB stars, from the cores of AGB stars to presolar dust Lebzelter Thomas Institut für Astrophysik Stellar Wind Accretion and Raman O VI Spectroscopy of the Symbiotic Star AG Draconis Lee Young-Min Department of Physics and Astronomy, Sejong University Search for technetium and s-process elements in binary central stars of planetary nebulae Löbling Lisa European Southern Observatory Properties of OH/IR stars versus YSOs in mid- and far-infrared surveys Loup Cecile Observatoire Astronomique de Strasbourg, CNRS ZOOMING INTO THE COMPLEX DUSTY ENVELOPES OF C-RICH AGB STARS Lykou Foteini The University of Hong Kong Mass Loss Rates of Li-rich AGB/RGB Stars Maciel Walter University of Sao Paulo, Astronomy Department Observational constraints on thermal pulses and the evolution of the mass-loss rate Maercker Matthias Onsala Space Observatory Phase-lag measurements in dust-scattered, polarised light: the distance to R Scl Maercker Matthias Onsala Space Observatory The submm properties of dust in the detached shells around carbon AGB stars Maercker Matthias Onsala Space Observatory The interaction of the Helix nebula with the interstellar medium; a solid case. Manchado Arturo IAC The abundance of SiC2 in Carbon Star Envelopes Massalkhi Sarah Instituto de Física Fundamental, CSIC Separation of gas and dust in the winds of AGB stars Mattsson Lars Nordita, Stockholm University Mass-loss from solar-like and metal-poor stars McDonald Iain University of Manchester Modelling the extended dust emission around carbon stars observed by Herschel Mecina Marko Institut für Astrophysik Rotating stellar models of low- and intermediate-mass stars from the pre-main sequence up to the AGB Mendes Luiz Themystokliz SanctosUniversidade Federal de Minas Gerais A common-envelope wind model for SNe Ia Meng Xiangcun Yunnan Observatories/CAS Long Period Variables in dwarf Irregular Galaxies of the Local Group Menzies John SAAO Impact of AGB stars on their circumstellar environments Mohamed Shazrene South African Astronomical Observatory A possible cross diagnosis for studying the convection on red supergiant stars Montargès Miguel KU Leuven Updates on the Ultraviolet Emission from Asymptotic Giant Branch Stars Montez Rodolfo Smithsonian Astrophysical Observatory Astrometric VLBI observation of the Galactic LPVs with VERA; Miras and OH/IR stars Nakagawa Akiharu Kagoshima University Carbon stars in the Magellanic Clouds: properties and dust production rate Nanni Ambra University of Padova, physics and astronomy department Near-infrared polarimetry of M2-9 Navarro Silvana G. IAM - Universidad de Guadalajara SMA Spectral Line Survey of the Proto-Planetary Nebula CRL 618 Nimesh Patel Harvard-Smithsonian Center for Astrophysics An episodic maser jet in the water fountain IRAS 18113-2503 Orosz Gabor Xinjiang Astronomical Observatory SWAG: Distribution and Kinematics of an Obscured AGB Population toward the Galactic Center Ott Juergen National Radio Astronomy Observatory Studying the large-amplitude optical variabilty of V648 Car Palma Tali Observatorio Astronómico, Universidad Nacional de Córdoba Calibrating TP-AGB stellar models and chemical yields through resolved stellar populations in the Small Magellanic Cloud Pastorelli Giada Dept. of Physics and Astronomy, Padova University AGB stars of the Magellanic Clouds as seen within the Delta-a photometric system Paunzen Ernst DTPA, Masaryk University AGB stars of the Magellanic Clouds as seen within the Delta-a photometric system Paunzen Ernst Institut für Astrophysik On the circumstellar effects on the Li and Ca abundances in massive Galactic AGB stars Pérez-Mesa Víctor Instituto de Astrofísica de Canarias AGB star atmospheres modeling, as feedback to stellar evolutionary and galaxy models Rau Gioia NASA/Goddard Space Flight Center Circumstellar Molecular Maser Emission of AGB and Post-AGB Stars Rudnitskij Georgij Sternberg Astronomical Institute High angular-resolution infrared imaging and spectra of the carbon-rich AGB star V Hya Sahai Raghvendra Jet Propulsion Laboratory Infrared Studies of the Variability and Mass Loss of Some of the Dustiest Asymptotic Giant Branch Stars in the Magellanic Clouds Sargent Benjamin Space Telescope Science Institute Observing the mass-loss of nearby red supergiants through high-contrast imaging Scicluna Peter ASIAA The Nearby Evolved Stars Survey: Project description and initial results Scicluna Peter ASIAA The temporal evolution of neutron-capture elements in the Galactic discs Spina Lorenzo Monash University Modelling circumstellar gas and dust in Magellanic Cloud and Galactic carbon stars Srinivasan Sundar Institute of Astronomy & Astrophysics, Academia Sinica Modelling dust in the Nearby Evolved Star Survey (NESS) targets Srinivasan Sundar Institute of Astronomy & Astrophysics, Academia Sinica Population of AGB stars in the Outer Galaxy Szczerba Ryszard Nicolaus Copernicus Astronomical Center The role of asymptotic giant branch stars in the chemical evolution of the Galaxy Tautvaisiene Grazina Vilnius University New limit on delta alpha/alpha from an analysis QSO spectra Thong Le Institute for Computational Science The star formation history in the M31 galaxy derived from Long-Period-Variable star counts Torki Maryam University of zanjan Characterisation of Long Period Variables in the Magellanic Clouds Trabucchi Michele University of Padova - Department of Physics and Astronomy Dust-production of AGB stars in the Solar Neighborhood Trejo Alfonso ASIAA Comprehensive analyses of panchromatic data sets and photo-ionization modeling of PNe Ueta Toshiya Univ. of Denver Excavating Mass Loss History in Extended Dust Shells of Evolved Stars (MLHES): AKARI Mission Programme Ueta Toshiya Univ. of Denver Herschel Planetary Nebula Survey Plus (HerPlaNS+) Ueta Toshiya Univ. of Denver Morpho-Kinematics of the Circumstellar Environments around Post-AGB Stars Ueta Toshiya Univ. of Denver Planetary Nebulae detected in the AKARI Far-IR All-Sky Survey Maps Ueta Toshiya Univ. of Denver Dust Structure around Asymptotic Giant Branch Stars Upadhyay Devendra Raj Amrit Campus (ASCOL), Tribhuvan University We determine the distance 91 longer period Mira variables using 3.4µm Period Luminosity Relation Urago Riku Kagoshima University Looking for new water-fountain stars Uscanga Lucero University of Guanajuato The interplay between pulsation, mass loss, and third dredge-up: More about Miras with and without technetium Uttenthaler Stefan Kuffner Sternwarte Determining the effect of a non-uniform AGB outflow on its chemistry Van de Sande Marie KU Leuven Spectroscopic variability of proto-planetary nebulae Van de Steene Griet Royal Observatory of Brussels Circumstellar chemistry of Si-C bearing molecules in the C-rich AGB star IRC+10216 Velilla-Prieto Luis Instituto de Física Fundamental (CSIC) Measuring spatially resolved gas-to-dust ratios in AGB stars Wallstrom Sofia ASIAA WD+AGB star as the progenitors of type Ia supernovae Wang Bo Yunnan Observatories, Chinese Academy of Sciences K-Type Supergiants in the Large Magellanic Cloud Wing Robert Ohio State University A carbon star sheds its skin Wittkowski Markus ESO TIGvival -- High-resolution spectroscopic monitoring of long-period variables using TIGRE Wolter Uwe Hamburger Sternwarte Models of binaries containing giants Yakut Kadri University of EGE