2011AJ....141..155J


Query : 2011AJ....141..155J

2011AJ....141..155J - Astron. J., 141, 155 (2011/May-0)

An upper bound to the space density of interstellar comets.

JURA M.

Abstract (from CDS):

Two well-studied white dwarfs with helium-dominated atmospheres (DBs) each possess less hydrogen than carried by a single average-mass comet. Plausibly, the wind rates from these stars are low enough that most accreted hydrogen remains with the star. If so, and presuming their nominal effective temperatures, then these DBs have faced minimal impact by interstellar comets during their 50 Myr cooling age; interstellar iceballs with radii between 10 m and 2 km contain less than 1% of all interstellar oxygen. This analysis suggests that most stars do not produce comets at the rate predicted by "optimistic" scenarios for the formation of the Oort Cloud.

Abstract Copyright: ∼

Journal keyword(s): ISM: general - planetary systems - white dwarfs

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 - 2026
#notes
1 EGGR 409 WD* 01 14 37.6538960064 +10 41 04.757053956   15.27 15.41 15.69   DB2.5 75 0
2 GD 40 WD* 03 02 53.1037481136 -01 08 33.798683976   15.479 15.384     DBZ4 187 0
3 WG 7 WD* 03 09 47.9177537304 -56 23 49.411222764   13.99 14.14 14.42   DB 59 0
4 GALEX J122859.9+104032 WD* 12 28 59.9341604496 +10 40 33.045988944           DAZe: 152 0
5 GD 190 WD* 15 44 19.4543884752 +18 06 43.775072424 13.537 14.556 14.677 14.767 14.849 DB2 94 0
6 GD 358 WD* 16 47 18.3925183824 +32 28 32.862804384 12.511 13.530 13.653 13.752 13.852 DB2 364 0
7 V* QU Tel WD* 20 09 40.1871967824 -52 25 15.864452508 14.51 15.25 15.03     DB2 60 1
8 PG 2354+159 WD* 23 56 34.7462697000 +16 15 40.257339876   15.78   16.15   DBZ 30 0

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