2025A&A...698A.138B


Query : 2025A&A...698A.138B

2025A&A...698A.138B - Astronomy and Astrophysics, volume 698A138 (2025/6-1)

Interstellar dust measured in situ by Ulysses: New aspects of the particle size distribution and its modulation by the heliosheath.

BAALMANN L.R., JANISCH T., HUNZIKER S., STRUB P., KRUGER H., HOFSTETTER K., SIEBER M. and STERKEN V.J.

Abstract (from CDS):

Interstellar dust (ISD) enters the heliosphere from the direction of its nose. It is first modulated by the heliosheath and then the inner heliosphere before it is measured by the dust detectors on board of spacecraft, for example on Ulysses. Various criteria exist to distinguish ISD from the dust of other sources, and different methods exist to determine the particle masses and impact speeds from the measurements.

Abstract Copyright: © The Authors 2025

Journal keyword(s): Sun: heliosphere - interplanetary medium - dust - extinction - ISM: general

Simbad objects: 3

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Number of rows : 3
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 NAME G Cloud Cld 03 00 +50.2           ~ 85 0
2 NAME LIC Cld 04 41 +31.           ~ 317 0
3 * eps CMa * 06 58 37.54876 -28 58 19.5102 0.36 1.29 1.50 1.59 1.80 B1.5II 519 0

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