2019A&A...627A..77M


Query : 2019A&A...627A..77M

2019A&A...627A..77M - Astronomy and Astrophysics, volume 627A, 77-77 (2019/7-1)

ISPY - NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring.

MUSSO BARCUCCI A., LAUNHARDT R., KENNEDY G.M., AVENHAUS H., BREMS S.S., VAN BOEKEL R., CANTALLOUBE F., CHEETHAM A., CUGNO G., GIRARD J., GODOY N., HENNING T.K., METCHEV S., MULLER A., OLOFSSON J., PEPE F., QUANZ S.P., QUIRRENBACH A., REFFERT S., RICKMAN E.L., SAMLAND M. and SEGRANSAN D.

Abstract (from CDS):

Context. The interaction between low-mass companions and the debris discs they reside in is still not fully understood. A debris disc can evolve due to self-stirring, a process in which planetesimals can excite their neighbours to the point of destructive collisions. In addition, the presence of a companion could further stir the disc (companion-stirring). Additional information is necessary to understand this fundamental step in the formation and evolution of a planetary system, and at the moment of writing only a handful of systems are known where a companion and a debris disc have both been detected and studied at the same time. Aims. Our primary goal is to augment the sample of these systems and to understand the relative importance between self-stirring and companion-stirring. Methods. In the course of the VLT/NaCo Imaging Survey for Planets around Young stars (ISPY), we observed HD 193571, an A0 debris disc hosting star at a distance of 68pc with an age between ∼60 and 170Myr. We obtained two sets of observations in L' band and a third epoch in H band using the GPI instrument at Gemini-South. Results. A companion was detected in all three epochs at a projected separation of ∼11au (∼0.17''), and co-motion was confirmed through proper motion analysis. Given the inferred disc size of 120au, the companion appears to reside within the gap between the host star and the disc. Comparison between the L' and H band magnitude and evolutionary tracks suggests a mass of ∼0.31-0.39M. Conclusions. We discovered a previously unknown M-dwarf companion around HD 193571, making it the third low-mass stellar object discovered within a debris disc. A comparison to self- and companion-stirring models suggests that the companion is likely responsible for the stirring of the disc.

Abstract Copyright: © A. Musso Barcucci et al. 2019

Journal keyword(s): stars: individual: HD 193571 - planet-disk interactions - planets and satellites: detection - infrared: planetary systems - instrumentation: high angular resolution - techniques: high angular resolution

VizieR on-line data: <Available at CDS (J/A+A/627/A77): list.dat fits/*>

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 HD 50571 PM* 06 50 01.0151260800 -60 14 56.921260776   6.548 6.098 7.26   F5VFe+0.4 84 0
2 HD 95086 * 10 57 03.0215719872 -68 40 02.449216128   7.60 7.36     A8III 171 1
3 * kap01 Sgr PM* 20 22 27.5022576960 -42 02 58.423208352 5.59 5.59 5.59     A0V 86 0
4 HD 193571B Pl? 20 22 27.5022576960 -42 02 58.423208352           ~ 1 0
5 HD 206893 PM* 21 45 21.9052532928 -12 47 00.060804636   7.11 6.67     F5V 106 0
6 HD 218396 El* 23 07 28.7157209544 +21 08 03.310767492   6.21 5.953     F0+VkA5mA5 1115 0

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2023.11.28-15:12:22

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