2011A&A...536L...4E


Query : 2011A&A...536L...4E

2011A&A...536L...4E - Astronomy and Astrophysics, volume 536, L4-4 (2011/12-1)

Herschel discovery of a new class of cold, faint debris discs.

EIROA C., MARSHALL J.P., MORA A., KRIVOV A.V., MONTESINOS B., ABSIL O., ARDILA D., AREVALO M., AUGEREAU J.-C., BAYO A., DANCHI W., DEL BURGO C., ERTEL S., FRIDLUND M., GONZALEZ-GARCIA B.M., HERAS A.M., LEBRETON J., LISEAU R., MALDONADO J., MEEUS G., MONTES D., PILBRATT G.L., ROBERGE A., SANZ-FORCADA J., STAPELFELDT K., THEBAULT P., WHITE G.J. and WOLF S.

Abstract (from CDS):

We present Herschel PACS 100 and 160µm observations of the solar-type stars α Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel open time key programme (OTKP) DUNES (DUst around NEarby Stars). Our observations show small infrared excesses at 160µm for all three stars. HD 210277 also shows a small excess at 100µm, while the 100µm fluxes of α Men and HD 88230 agree with the stellar photospheric predictions. We attribute these infrared excesses to a new class of cold, faint debris discs. Both α Men and HD 88230 are spatially resolved in the PACS 160 µm images, while HD 210277 is point-like at that wavelength. The projected linear sizes of the extended emission lie in the range from ∼115 to ≤250AU. The estimated black body temperatures from the 100 and 160µm fluxes are ≲22K, and the fractional luminosity of the cold dust is Ldust/L*∼10–6, close to the luminosity of the solar-system's Kuiper belt. These debris discs are the coldest and faintest discs discovered so far around mature stars, so they cannot be explained easily invoking ``classical'' debris disc models.

Abstract Copyright:

Journal keyword(s): circumstellar matter - planetary systems - stars: individual: {alpha} Men (HIP 29271) - stars: individual: HD 88230 - stars: individual: HD 210277

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 * alf Men PM* 06 10 14.4725823672 -74 45 10.958331816   5.798 5.069     G7V 273 0
2 HD 88230 Er* 10 11 22.1399492383 +49 27 15.251007087 9.23 7.94 6.61 5.36 4.56 K6VeFe-1 457 0
3 HD 207129 PM* 21 48 15.7511634187 -47 18 13.017893348   6.18 5.58     G2V 325 0
4 HD 210277 PM* 22 09 29.8657847411 -07 32 55.162082226   8.85 8.57 7.36   G8V 334 1
5 * alf PsA PM* 22 57 39.04625 -29 37 20.0533 1.31 1.25 1.16 1.11 1.09 A4V 1216 3

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2023.09.29-16:05:52

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