Article (Scientific journals)
Exocomets: A spectroscopic survey
Rebollido, I.; Eiroa, C.; Montesinos, B. et al.
2020In Astronomy and Astrophysics, 639, p. 11
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Keywords :
stars: general; comets: general; Kuiper belt: general; ISM: clouds; Astrophysics - Solar and Stellar Astrophysics; Astrophysics - Earth and Planetary Astrophysics; Astrophysics - Astrophysics of Galaxies
Abstract :
[en] Context. While exoplanets are now routinely detected, the detection of small bodies in extrasolar systems remains challenging. Since the discovery of sporadic events, which are interpreted to be exocomets (falling evaporating bodies) around β Pic in the early 1980s, only ∼20 stars have been reported to host exocomet-like events. <BR /> Aims: We aim to expand the sample of known exocomet-host stars, as well as to monitor the hot-gas environment around stars with previously known exocometary activity. <BR /> Methods: We have obtained high-resolution optical spectra of a heterogeneous sample of 117 main-sequence stars in the spectral type range from B8 to G8. The data were collected in 14 observing campaigns over the course of two years from both hemispheres. We analysed the Ca II K&H and Na I D lines in order to search for non-photospheric absorptions that originated in the circumstellar environment and for variable events that could be caused by the outgassing of exocomet-like bodies. <BR /> Results: We detected non- photospheric absorptions towards 50% of the sample, thus attributing a circumstellar origin to half of the detections (i.e. 26% of the sample). Hot circumstellar gas was detected in the metallic lines inspected via narrow stable absorptions and/or variable blue- and red-shifted absorption events. Such variable events were found in 18 stars in the Ca II and/or Na I lines; six of them are reported in the context of this work for the first time. In some cases, the variations we report in the Ca II K line are similar to those observed in β Pic. While we do not find a significant trend in the age or location of the stars, we do find that the probability of finding CS gas in stars with larger v sin i is higher. We also find a weak trend with the presence of near-infrared excess and with anomalous (λ Boo-like) abundances, but this would require confirmation by expanding the sample. <P />Table C.1 is only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr/">http://cdsarc.u-strasbg.fr</A> (ftp://130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz- bin/cat/J/A+A/639/A11">http://cdsarc.u-strasbg.fr/viz- bin/cat/J/A+A/639/A11</A>
Research center :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Rebollido, I.;  Dpto. Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049, Madrid, Spain
Eiroa, C.;  Dpto. Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049, Madrid, Spain ; Observatorio Astrónomico de Calar Alto, CAHA, 04550, Gérgal, Almería, Spain
Montesinos, B.;  Centro de Astrobiología (CAB, CSIC-INTA), ESAC Campus Camino Bajo del Castillo, s/n, Villanueva de la Cañada, 28692, Madrid, Spain
Maldonado, J.;  INAF, Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy
Villaver, E.;  Dpto. Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049, Madrid, Spain
Absil, Olivier  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > PSILab
Bayo, A.;  Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, 5030, Casilla, Valparaíso, Chile ; Núcleo Milenio de Formación Planetaria - NPF, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
Canovas, H.;  European Space Astronomy Centre (ESA), PO Box 78, 28691, Villanueva de la Cañada, Madrid, Spain
Carmona, A.;  Université de Toulouse, UPS-OMP, IRAP, Toulouse, 31400, France
Chen, Ch;  Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, 21212, USA
Ertel, S.;  Steward Observatory, Department of Astronomy, University of Arizona, Tucson, AZ, 85721, USA
Henning, Th;  Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117, Heidelberg, Germany
Iglesias, D. P.;  Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, 5030, Casilla, Valparaíso, Chile ; Núcleo Milenio de Formación Planetaria - NPF, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
Launhardt, R.;  Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117, Heidelberg, Germany
Liseau, R.;  Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, 439 92, Onsala, Sweden
Meeus, G.;  Dpto. Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049, Madrid, Spain
Moór, A.;  Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Konkoly-Thege Miklós út 15-17, 1121, Budapest, Hungary ; ELTE Eötvös Loránd University, Institute of Physics, Pázmány Péter sétány 1/A, 1117, Budapest, Hungary
Mora, A.;  Aurora Technology B.V. for ESA, ESA-ESAC, Villanueva de la Cañada, 28691, Madrid, Spain
Olofsson, J.;  Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, 5030, Casilla, Valparaíso, Chile ; Núcleo Milenio de Formación Planetaria - NPF, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
Rauw, Grégor  ;  Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Riviere-Marichalar, P.;  Observatorio Astronómico Nacional (OAN-IGN)-Observatorio de Madrid, Alfonso XII, 3, 28014, Madrid, Spain)
More authors (11 more) Less
Language :
English
Title :
Exocomets: A spectroscopic survey
Publication date :
01 July 2020
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
639
Pages :
A11
Peer reviewed :
Peer Reviewed verified by ORBi
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