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An Unbiased SPHERE-IFS Survey of Nearby Herbig Ae/Be Stars: Are All Group I Disks Transitional?

Published online by Cambridge University Press:  13 January 2020

Maria Giulia Ubeira Gabellini
Affiliation:
Dip. di Fisica, Universitá Degli Studi di Milano, Via Celoria, 16, Milano, I-20133, Italy email: [email protected], [email protected] ESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany email: [email protected], [email protected]
Mario E. van den Ancker
Affiliation:
ESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany email: [email protected], [email protected]
Davide Fedele
Affiliation:
INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy email: [email protected]
Giuseppe Lodato
Affiliation:
Dip. di Fisica, Universitá Degli Studi di Milano, Via Celoria, 16, Milano, I-20133, Italy email: [email protected], [email protected]
Carlo Felice Manara
Affiliation:
ESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, Germany email: [email protected], [email protected]
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Abstract

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Using a novel method for speckle noise suppression from SPHERE-IFS data, we performed a systematic survey for disks in 22 Herbig Ae/Be stars, spatially resolving five disks and detecting seven new companion candidates. The fraction of sources with spatially resolved disks is systematically higher in the Meeus et al. (2001) group I sources, showing that disks are indeed more easily seen in scattered light in this sub-class of Herbig stars, consistent with the interpretation of group I sources having large gaps in their disks.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020 

References

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