output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

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astro-ph.HE2023

Polarised light from accreting low mass X-ray binaries

F. Capitanio, A. Gnarini, S. Fabiani +5

Thanks to IXPE , the X-ray spectro-polarimeter launched at the end of 2021, X-ray polarimetry has finally become an extraordinary tool in investigating the physics of accretion in…

astro-ph.SR2023★ 1 cited

The He abundance in NGC 1850 A and B: are we observing the early stage of formation of multiple populations in a stellar cluster?

R. Carini, A. Sollima, E. Brocato +1

We present the result of a sample of B-stars in the Large Magellanic Cloud young double stellar cluster NGC 1850 A and NGC 1850 B, observed with the integral-field spectrograph at…

astro-ph.SR2023★ 1 cited

Seismic and spectroscopic analysis of 9 bright red giants observed by Kepler

H. R. Coelho, A. Miglio, T. Morel +21

Photometric time series gathered by space telescopes such as CoRoT and Kepler allow to detect solar-like oscillations in red-giant stars and to measure their global seismic constra…

astro-ph.HE2023

Swift/XRT observations of superorbital modulations in wind-fed supergiant X-ray binaries

P. Romano, E. Bozzo, N. Islam +1

We present the first Swift/XRT long-term monitoring of 2S 0114+650, a wind-fed supergiant X-ray binary for which both orbital and superorbital periods are known (P_orb~11.6d and P_…

astro-ph.GA2023★ 40 cited

Nebular emission from young stellar populations including binary stars

M. Lecroq, S. Charlot, A. Bressan +8

We investigate the nebular emission produced by young stellar populations using the new GALSEVN model based on the combination of the SEVN population-synthesis code including binar…

astro-ph.GA2023

Jeans modelling of weakly flattened stellar systems

Antonio Mancino, Luca Ciotti, Silvia Pellegrini +1

In the homoeoidal expansion, a given ellipsoidally stratified density distribution, and its associated potential, are expanded in the (small) density flattening parameter , and…