2010A&A...518L.131E


Query : 2010A&A...518L.131E

2010A&A...518L.131E - Astronomy and Astrophysics, volume 518, L131-131 (2010/7-2)

Cold DUst around NEarby stars (DUNES). First results. A resolved exo-Kuiper belt around the solar-like star ζ2 Ret.

EIROA C., FEDELE D., MALDONADO J., GONZALEZ-GARCIA B.M., RODMANN J., HERAS A.M., PILBRATT G.L., AUGEREAU J.-C., MORA A., MONTESINOS B., ARDILA D., BRYDEN G., LISEAU R., STAPELFELDT K., LAUNHARDT R., SOLANO E., BAYO A., ABSIL O., AREVALO M., BARRADO D., BEICHMAN C., DANCHI W., DEL BURGO C., ERTEL S., FRIDLUND M., FUKAGAWA M., GUTIERREZ R., GRUEN E., KAMP I., KRIVOV A., LEBRETON J., LOEHNE T., LORENTE R., MARSHALL J., MARTINEZ-ARNAIZ R., MEEUS G., MONTES D., MORBIDELLI A., MUELLER S., MUTSCHKE H., NAKAGAWA T., OLOFSSON G., RIBAS I., ROBERGE A., SANZ-FORCADA J., THEBAULT P., WALKER H., WHITE G.J. and WOLF S.

Abstract (from CDS):

We present the first far-IR observations of the solar-type stars δ Pav, HR 8501, 51 Peg and ζ2 Ret, taken within the context of the DUNES Herschel open time key programme (OTKP). This project uses the PACS and SPIRE instruments with the objective of studying infrared excesses due to exo-Kuiper belts around nearby solar-type stars. The observed 100 µm fluxes from δ Pav, HR 8501, and 51 Peg agree with the predicted photospheric fluxes, excluding debris disks brighter than Ldust/L*∼5x10–7 (1σ level) around those stars. A flattened, disk-like structure with a semi-major axis of ∼100AU in size is detected around ζ2 Ret. The resolved structure suggests the presence of an eccentric dust ring, which we interpret as an exo-Kuiper belt with Ldust/L*≃10–5.

Abstract Copyright:

Journal keyword(s): stars: general - planetary system - space vehicles: instruments

Simbad objects: 8

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Number of rows : 8
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 * q01 Eri PM* 01 42 29.3145176952 -53 44 26.991453264   6.05 5.52     F9V 325 1
2 * zet02 Ret ** 03 18 12.8188824117 -62 30 22.904711032   5.814 5.228     G1V 362 0
3 HD 61005 PM* 07 35 47.4623556456 -32 12 14.045086368   8.96 8.22     G8Vk 228 0
4 * alf Boo RG* 14 15 39.67207 +19 10 56.6730 2.46 1.18 -0.05 -1.03 -1.68 K1.5IIIFe-0.5 2322 1
5 * del Pav PM* 20 08 43.6088716052 -66 10 55.442769229 4.78 4.32 3.56 2.95 2.61 G8IV 391 0
6 HD 211415 PM* 22 18 15.6133953371 -53 37 37.466806476   5.98 5.39 6.52   G0V 194 0
7 * 51 Peg PM* 22 57 27.9804852576 +20 46 07.797040104 6.39 6.16 5.46 4.97 4.61 G2IV 1160 1
8 * alf PsA PM* 22 57 39.04625 -29 37 20.0533 1.31 1.25 1.16 1.11 1.09 A4V 1236 3

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