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  5. The triple system AT Mic AB + AU Mic in the β Pictoris association
 

The triple system AT Mic AB + AU Mic in the β Pictoris association

Journal
ASTROPHYSICS AND SPACE SCIENCE  
Date Issued
2016
Author(s)
MESSINA, Sergio  
•
LETO, Giuseppe  
•
PAGANO, Isabella  
DOI
10.1007/s10509-016-2886-x
Abstract
Equal-mass stars in young open clusters and loose associations exhibit a wide spread of rotation periods, which likely originates from differences in the initial rotation periods and in the primordial disc lifetimes. We want to explore if the gravitational effects by nearby companions may play an additional role in producing the observed rotation period spread, as well as, the role that magnetic activity may also play. We measure the photometric rotation periods of components of multiple stellar systems and look for correlations of the period differences among the components to their reciprocal distances. In this paper, we analyzed the triple system AU Mic + AT Mic A&B in the 25± 3-Myr β Pictoris association. We have retrieved from the literature the rotation period of AU Mic ({P} = 4.85 d) and measured from photometric archival data the rotation periods of both components of AT Mic ({P} = 1.19 d and {P} = 0.78 d) for the first time. Moreover, we detected a high rate of flare events from AT Mic. Whereas the distant component AU Mic has evolved rotationally as a single star, the A and B components of AT Mic, separated by ∼ 27 AU, exhibit a rotation rate a factor 5 larger than AU Mic. Moreover, the A and B components, despite have about equal mass, show a significant difference (∼ 40 %) between their rotation periods. A possible explanation is that the gravitational forces between the A and B components of AT Mic (that are a factor ∼ 7.3× 106 more intense than those between AU Mic and AT Mic) have enhanced the dispersal of the AT Mic primordial disc, shortening its lifetime and the disc-locking phase duration, making the component A and B of AT Mic to rotate faster than the more distant AU Mic. We suspect that a different level of magnetic activity between the A and B components of AT Mic may be the additional parameter responsible for the difference between their rotation periods.
Volume
361
Issue
9
Start page
291
Uri
http://hdl.handle.net/20.500.12386/24451
Url
https://link.springer.com/article/10.1007/s10509-016-2886-x
Issn Identifier
0004-640X
Ads BibCode
2016Ap&SS.361..291M
Rights
open.access
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