SIMBAD references

2019MNRAS.484L..38M - Mon. Not. R. Astron. Soc., 484, L38-L42 (2019/March-3)

Time-resolved image polarimetry of TRAPPIST-1 during planetary transits.

MILES-PAEZ P.A., ZAPATERO OSORIO M.R., PALLE E. and METCHEV S.A.

Abstract (from CDS):

We obtained linear polarization photometry (J-band) and low-resolution spectroscopy (ZJ-bands) of TRAPPIST-1, which is a planetary system formed by an M8-type low-mass star and seven temperate, Earth-sized planets. The photopolarimetric monitoring campaign covered 6.5 h of continuous observations including one full transit of planet TRAPPIST-1d and partial transits of TRAPPIST-1b and e. The spectrophotometric data and the photometric light curve obtained over epochs with no planetary transits indicate that the low-mass star has very low level of linear polarization compatible with a null value. However, the 'in transit' observations reveal an enhanced linear polarization signal with peak values of p*=0.1 per cent^ with a confidence level of 3σ, particularly for the full transit of TRAPPIST-1d, thus confirming that the atmosphere of the M8-type star is very likely dusty. Additional observations probing different atmospheric states of TRAPPIST-1 are needed to confirm our findings, as the polarimetric signals involved are low. If confirmed, polarization observations of transiting planetary systems with central ultracool dwarfs can become a powerful tool for the characterization of the atmospheres of the host dwarfs and the validation of transiting planet candidates that cannot be corroborated by any other method.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): polarization - stars: atmospheres - stars: individual: TRAPPIST-1 - stars: late-type - stars: low-mass

Simbad objects: 8

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2021.06.21-00:09:34

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