STARKEY - Publications

Check the complete list of STARKEY-supported publications on ADS

• Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud. Pastorelli et al. 2020, eprint arXiv:2008.08595
• PHAT XX. AGB stars and other cool giants in M31 star clusters. Girardi et al. 2020, eprint arXiv:2008.07184
• YBC: a stellar bolometric corrections database with variable extinction coefficients. Application to PARSEC isochrones. Chen et al. 2020, A&A, 632, 105
• Carbon star formation as seen through the non-monotonic initial-final mass relation. Marigo et al. 2020, Nature Astronomy,
• Period-luminosity diagram of long period variables in the Magellanic Clouds. New aspects revealed from Gaia Data Release 2. Lebzelter et al. 2019, A&A, 631, 24
• Carbon stars with increased oxygen and nitrogen abundances: hydrostatic dust-free model atmospheres. Aringer et al. 2019, MNRAS, 487, 2133
• The mass-loss, expansion velocities, and dust production rates of carbon stars in the Magellanic Clouds. Nanni et al. 2019, MNRAS, 487, 502
• Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud. Pastorelli et al. 2019, MNRAS, 485, 5666
• The onset of the AGB wind tied to a transition between sequences in the period-luminosity diagram. McDonald & Trabucchi 2019, MNRAS, 484, 4678
• Carbon star wind models at solar and sub-solar metallicities: a comparative study. I. Mass loss and the properties of dust-driven winds. Bladh et al. 2019, A&A, 623, A119
• Optical properties of amorphous carbon dust around C-stars: new constraints from 2MASS and Gaia observations. Nanni 2019, MNRAS, 482, 4726
• Modelling long-period variables - I. A new grid of O-rich and C-rich pulsation models. Trabucchi et al. 2019, MNRAS, 482, 929
• The VMC survey - XXXI: The spatially resolved star formation history of the main body of the Small Magellanic Cloud. Rubele et al. 2018, MNRAS, 478, 5017
• A new method to identify subclasses among AGB stars using Gaia and 2MASS photometry. Lebzelter et al. 2018, A&A, 616, L13
• Estimating the dust production rate of carbon stars in the Small Magellanic Cloud. Nanni et al. 2018, MNRAS, 473, 5492
• A New Interpretation of the Period-Luminosity Sequences of Long-period Variables. Trabucchi et al. 2017, ApJ, 847, 139
• Tomography of silicate dust around M-type AGB stars. I. Diagnostics based on dynamical models. Bladh et al. 2017, A&A, 607, A27
• A New Generation of PARSEC-COLIBRI Stellar Isochrones Including the TP-AGB Phase. Marigo et al. 2017, ApJ, 835, 77
• Constraining dust properties in circumstellar envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of carbon dust. Nanni et al. 2016, MNRAS, 462, 1215
• Synthetic photometry for M and K giants and stellar evolution: hydrostatic dust-free model atmospheres and chemical abundances. Aringer et al. 2016, MNRAS, 457, 3611
• Connecting the evolution of thermally pulsing asymptotic giant branch stars to the chemistry in their circumstellar envelopes - I. Hydrogen cyanide. Marigo et al. 2016, MNRAS, 456, 23
• The VMC survey - XIV. First results on the look-back time star formation rate tomography of the Small Magellanic Cloud. Rubele et al. 2015, MNRAS, 449, 639
• Exploring wind-driving dust species in cool luminous giants. III. Wind models for M-type AGB stars: dynamic and photometric properties. Bladh et al. 2015, A&A, 575, A105