2010ApJ...714.1386F


Query : 2010ApJ...714.1386F

2010ApJ...714.1386F - Astrophys. J., 714, 1386-1397 (2010/May-2)

Strengthening the case for asteroidal accretion: evidence for subtle and diverse disks at white dwarfs.

FARIHI J., JURA M., LEE J.-E. and ZUCKERMAN B.

Abstract (from CDS):

Spitzer Space Telescope IRAC 3-8 µm and AKARI IRC 2-4 µm photometry are reported for 10 white dwarfs with photospheric heavy elements; nine relatively cool stars with photospheric calcium and one hotter star with a peculiar high carbon abundance. A substantial infrared excess is detected at HE 2221-1630, while modest excess emissions are identified at HE 0106-3253 and HE 0307+0746, implying these latter two stars have relatively narrow (Δr < 0.1 R ) rings of circumstellar dust. A likely 7.9 µm excess is found at PG 1225-079 and may represent, together with G166-58, a sub-class of dust ring with a large inner hole. The existence of attenuated disks at white dwarfs substantiates the connection between their photospheric heavy elements and the accretion of disrupted minor planets, indicating many polluted white dwarfs may harbor orbiting dust, even those lacking an obvious infrared excess.

Abstract Copyright:

Journal keyword(s): circumstellar matter - minor planets, asteroids: general - planetary systems - stars: abundances - white dwarfs

Simbad objects: 26

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Number of rows : 26
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 HS 0047+1903 WD* 00 50 12.4545315432 +19 19 48.512540388   15.94 15.59 16.0   DAZ 17 0
2 2MASS J01083497-3237486 * 01 08 34.9694649216 -32 37 48.581498388           ~ 1 0
3 Ton S 193 WD* 01 08 36.0345990648 -32 37 43.377234996   15.34 15.26 15.86   DAZ 30 0
4 Wolf 88 WD* 01 48 56.7965896608 +19 02 27.484961100   15.5   15.4   DAZB 55 0
5 GD 40 WD* 03 02 53.1037481136 -01 08 33.798683976   15.51 15.56     DBZ4 165 0
6 HS 0307+0746 WD* 03 10 09.1588178784 +07 57 32.073855264   17.1   16.6   DAZ 23 0
7 GD 56 WD* 04 11 02.1686667960 -03 58 22.586865708   15.64 15.50 15.1   DA3.3 75 0
8 HD 69830 PM* 08 18 23.9469682407 -12 37 55.817187530   6.74 5.95     G8:V 526 1
9 Ton 345 WD* 08 45 39.1819378488 +22 57 28.251061956   15.2 16.07     DB 74 0
10 GD 303 WD* 10 14 37.0860166680 +56 48 32.692906188   15.5       DBZ4 49 0
11 PG 1015+161 WD* 10 18 03.8273436048 +15 51 58.566029940   15.70   15.2   DA2.5 75 0
12 GALEX J104341.5+085558 WD* 10 43 41.5313708256 +08 55 58.340933400           DAZ 58 0
13 GD 133 WD* 11 19 12.3988618680 +02 20 33.045927216   14.76 14.57 14.8   DA4.0 87 0
14 EC 11507-1519 WD* 11 53 15.2581290960 -15 36 36.506488428   16.16 16.00 15.9   DA4.0 49 0
15 PG 1225-079 WD* 12 27 47.3585913504 -08 14 37.972720428   14.86 14.74 15.15   DZA4 70 0
16 GALEX J122859.9+104032 WD* 12 28 59.9341604496 +10 40 33.045988944           DAZe: 131 0
17 EGGR 298 WD* 14 58 06.4884482642 +29 37 29.515263565   15.86   15.3   DA6.8 89 0
18 PG 1457-086 WD* 14 59 52.9901145672 -08 49 29.645894676   15.68 15.77 15.8   DA2.3 44 0
19 GD 190 WD* 15 44 19.4543884752 +18 06 43.775072424 13.537 14.556 14.677 14.767 14.849 DB2 87 0
20 PG 1632+177 WD* 16 34 41.8477268232 +17 36 34.089084576   13.36 13.14 13.34   DA4.9 41 0
21 GD 205 WD* 17 11 55.6598934984 +23 01 01.525512072   14.81   15.1   DBAZ 40 0
22 GD 362 WD* 17 31 34.3168718112 +37 05 20.711767812   16.3   16.4   DAZB 175 0
23 LAWD 84 WD* 21 19 36.5325585235 -55 50 14.465412588 13.94 14.50 14.27 14.5   DA5.1 80 0
24 PHL 5103 WD* 22 24 17.4348213312 -16 15 47.161639476   16.30 16.02 16.25 15.90 DAZ 30 0
25 HS 2229+2335 WD* 22 31 45.4681881984 +23 51 23.355178596   16.02 16.01 16.37   DAZ 23 0
26 V* ZZ Psc WD* 23 28 47.6365087803 +05 14 54.235051503   13.17   13.0   DA4.1 484 0

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