output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2020 · astro-ph.SRShow all

36 papers · 2 filters

astro-ph.SR2020★ 30 cited

Understanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST

E. Marini, F. Dell'Agli, M. A. T. Groenewegen +6

Carbon stars have been and are extensively studied, given their complex internal structure and their peculiar chemical composition, which make them living laboratories to test stel…

astro-ph.SR2020★ 13 cited

Are extreme AGB stars post-common envelope binaries?

F. Dell'Agli, E. Marini, F. D'Antona +6

Modelling dust formation in single stars evolving through the carbon-star stage of the asymptotic giant branch (AGB) reproduces well the mid-infrared colours and magnitudes of most…

astro-ph.SR2020★ 56 cited

On the Use of Field RR Lyrae as Galactic Probes. II. A new S calibration to estimate their metallicity

J. Crestani, M. Fabrizio, V. F. Braga +33

We performed the largest and most homogeneous spectroscopic survey of field RR Lyraes (RRLs). We secured 6,300 high resolution (HR, R35,000) spectra for 143 RRLs (11…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.SR2020★ 17 cited

The Gaia spectrophotometric standard stars survey -- IV. Results of the absolute photometry campaign

G. Altavilla, S. Marinoni, E. Pancino +18

We present Johnson-Kron-Cousins BVRI photometry of 228 candidate spectrophotometric standard stars for the external (absolute) flux calibration of Gaia data. The data were gathered…

astro-ph.SR2020★ 8 cited

New insights into the use of Ultra Long Period Cepheids as cosmological standard candles

Ilaria Musella, Marcella Marconi, Roberto Molinaro +4

Ultra Long Period Cepheids (ULPs) are pulsating variable stars with a period longer than 80d and have been hypothesized to be the extension of the Classical Cepheids (CCs) at highe…