Query : 2017A&A...602L..10O

2017A&A...602L..10O - Astronomy and Astrophysics, volume 602, L10-10 (2017/6-1)

The inhomogeneous submillimeter atmosphere of Betelgeuse.


Abstract (from CDS):

The mechanisms responsible for heating the extended atmospheres of early-M spectral-type supergiants are poorly understood. So too is the subsequent role these mechanisms play in driving the large mass-loss rates of these stars. Here we present ALMA long (i.e., ∼16km) baseline 338GHz (0.89mm) continuum observations of the free-free emission in the extended atmosphere of the M2 spectral-type supergiant Betelgeuse. The spatial resolution of 14mas exquisitely resolves the atmosphere, revealing it to have a mean temperature of 2760K at ∼1.3R*, which is below both the photospheric effective temperature (Teff=3690K) and the temperatures at ∼2R*. This is unambiguous proof for the existence of an inversion of the mean temperature in the atmosphere of a red supergiant. The emission is clearly not spherically symmetric with two notable deviations from a uniform disk detected in both the images and visibilities. The most prominent asymmetry is located in the north-east quadrant of the disk and is spatially resolved showing it to be highly elongated with an axis-ratio of 2.4 and occupying ∼5% of the disk projected area. Its temperature is approximately 1000K above the measured mean temperature at 1.3R*. The other main asymmetry is located on the disk limb almost due east of the disk center and occupies ∼3% of the disk projected area. Both emission asymmetries are clear evidence for localized heating taking place in the atmosphere of Betelgeuse. We suggest that the detected localized heating is related to magnetic activity generated by large-scale photospheric convection.

Abstract Copyright: © ESO, 2017

Journal keyword(s): stars: atmospheres - stars: evolution - stars: imaging - stars: individual: Betelgeuse - submillimeter: stars - submillimeter: stars

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
1 QSO B0507+179 QSO 05 10 02.3689932504 +18 00 41.582562768   20.0 19.0 19.09   ~ 379 1
2 ICRF J055250.1+031327 Bz? 05 52 50.1013410696 +03 13 27.242707260       22.79   ~ 52 1
3 * 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 1568 0
4 ICRF J060510.1+093913 QSO 06 05 10.1131750728 +09 39 13.608958968           ~ 16 1
5 V* VY CMa s*r 07 22 58.32877 -25 46 03.2355 12.01 10.19 7.95     M5Iae 1056 0

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