2025A&A...700A.151P


Query : 2025A&A...700A.151P

2025A&A...700A.151P - Astronomy and Astrophysics, volume 700A151 (2025/8-1)

First images of the Antares photosphere from spectropolarimetry.

PILATE Q., JOSSELIN E., LEBRE A., LOPEZ ARISTE A., MATHIAS P. and LAVAIL A.

Abstract (from CDS):

Aims. Antares is the closest red supergiant (RSG) to Earth. The discovery of linear polarization in the atomic lines of the star opens the path to producing direct images of the photosphere, and hence probing the dynamics at the surface.
Methods. We analyze this linear polarization signals following the same scheme as has been previously done for the RSG Betelgeuse, and find that they are comparable in all its details. This allows us to use the same models for the analysis of these polarization signals in both stars.
Results. We find that, as in Betelgeuse, the linear polarization signal of Antares is due to the depolarization of the continuum, combined with brightness inhomogeneities. This allows us to produce images of the photosphere of the star. We show that in Antares convective cells can last several months and that the largest ones can occupy roughly 30% of the stellar radius.

Abstract Copyright: © The Authors 2025

Journal keyword(s): stars: individual: Antares - supergiants

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * 119 Tau s*r 05 32 12.7516308641 +18 35 39.251766506 8.63 6.41 4.33 2.55 1.13 M2Iab-Ib 295 0
2 * alf Ori s*r 05 55 10.30536 +07 24 25.4304 4.38 2.27 0.42 -1.17 -2.45 M1-M2Ia-Iab 1789 0
3 * alf Sco B Em* 16 29 24.20 -26 25 51.0   5.0 5.2     B2.5V 119 0
4 * alf Sco s*r 16 29 24.45970 -26 25 55.2094 4.08 2.75 0.91 -0.64 -1.87 M1.5Iab+B2Vn 786 0
5 * chi Cyg S* 19 50 33.9213430345 +32 54 50.575531294 7.02 6.06 4.24 1.81 -0.01 S6-9/1-2e 721 0
6 * mu. Cep s*r 21 43 30.4595558543 +58 46 48.165937434 8.85 6.43 4.08 1.98 0.22 M2-Ia 695 1

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