A near-infrared interferometric survey of debris-disk stars. IV. An unbiased sample of 92 southern stars observed in H band with VLTI/PIONIER

Ertel, S.; Absil, Olivier; Defrere, Denis; Le Bouquin, J.-B.; Augereau, J.-C.; Marion, Lindsay; Blind, N.; Bonsor, A.; Bryden, G.; Lebreton, J.; Milli, J.

doi:10.1051/0004-6361/201424438

Article (Périodiques scientifiques)

A near-infrared interferometric survey of debris-disk stars. IV. An unbiased sample of 92 southern stars observed in H band with VLTI/PIONIER

Ertel, S.; Absil, Olivier; Defrere, Denis et al.

2014 • In Astronomy and Astrophysics, 570, p. 128

Peer reviewed vérifié par ORBi

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https://hdl.handle.net/2268/173768

DOI
10.1051/0004-6361/201424438

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Mots-clés :

circumstellar matter; planetary systems; zodiacal dust

Résumé :

[en] Context. Detecting and characterizing circumstellar dust is a way to study the architecture and evolution of planetary systems. Cold dust in debris disks only traces the outer regions. Warm and hot exozodiacal dust needs to be studied in order to trace regions close to the habitable zone. <BR /> Aims: We aim to determine the prevalence and to constrain the properties of hot exozodiacal dust around nearby main-sequence stars. <BR /> Methods: We searched a magnitude-limited (H <= 5) sample of 92 stars for bright exozodiacal dust using our VLTI visitor instrument PIONIER in the H band. We derived statistics of the detection rate with respect to parameters, such as the stellar spectral type and age or the presence of a debris disk in the outer regions of the systems. We derived more robust statistics by combining our sample with the results from our CHARA/FLUOR survey in the K band. In addition, our spectrally dispersed data allowed us to put constraints on the emission mechanism and the dust properties in the detected systems. <BR /> Results: We find an overall detection rate of bright exozodiacal dust in the H band of 11% (9 out of 85 targets) and three tentative detections. The detection rate decreases from early type to late type stars and increases with the age of the host star. We do not confirm the tentative correlation between the presence of cold and hot dust found in our earlier analysis of the FLUOR sample alone. Our spectrally dispersed data suggest that either the dust is extremely hot or the emission is dominated by the scattered light in most cases. The implications of our results for the target selection of future terrestrial planet-finding missions using direct imaging are discussed.

Disciplines :

Aérospatiale, astronomie & astrophysique

Auteur, co-auteur :

Ertel, S.

Absil, Olivier ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)

Defrere, Denis

Le Bouquin, J.-B.

Augereau, J.-C.

Marion, Lindsay ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)

Blind, N.; Université de Liège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)

Bonsor, A.

Bryden, G.

Lebreton, J.

Milli, J.

Langue du document :

Anglais

Titre :

A near-infrared interferometric survey of debris-disk stars. IV. An unbiased sample of 92 southern stars observed in H band with VLTI/PIONIER

Date de publication/diffusion :

03 novembre 2014

Titre du périodique :

Astronomy and Astrophysics

ISSN :

0004-6361

eISSN :

1432-0746

Maison d'édition :

EDP Sciences, Les Ulis, France

Volume/Tome :

570

Pagination :

A128

Peer reviewed :

Peer reviewed vérifié par ORBi

URL complémentaire :

http://adsabs.harvard.edu/abs/2014A%26A...570A.128E

Disponible sur ORBi :

depuis le 11 novembre 2014

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