Incidence of debris discs around FGK stars in the solar neighbourhood

Incidence of debris discs around FGK stars in the solar neighbourhood

Context. Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their counterparts in the solar system are the asteroid and Edgeworth-Kuiper belts. Aims. The aim of this paper is to provide robust numbers for the incidence of debris di...

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Bibliographic Details
Main Authors: Montesinos, B., Eiroa, C., Krivov, A. V., Marshall, J. P., Pilbratt, G. L., Liseau, R., Mora, A., Maldonado, J., Wolf, S., Ertel, S., Bayo, A., Augereau, J.-C., Heras, A. M., Fridlund, M., Danchi, W. C., Solano, E., Kirchschlager, F., del Burgo, C., Montes, D.
Other Authors: Univ Arizona, Dept Astron, Steward Observ
Language:en
Published: EDP SCIENCES S A 2016
Subjects:
stars: late-type
circumstellar matter
protoplanetary disks
infrared: stars
Online Access:http://hdl.handle.net/10150/622160
http://arizona.openrepository.com/arizona/handle/10150/622160

Internet

http://hdl.handle.net/10150/622160
http://arizona.openrepository.com/arizona/handle/10150/622160

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