Luminosity Distance and Extinction by Submicrometer-sized Grains
The distance to the stars is a fundamental parameter, which is determined via two primary methods—parallax and luminosity. While the parallax is a direct trigonometric method, the luminosity distance is usually influenced by interstellar extinction. As long as the optical properties of dust grains a...
Saved in:
Main Authors: | R. Siebenmorgen, Frank Heymann, R. Chini |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/ada894 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Optical Extinction Law Depends on Magnetic Field Orientation: The RV–ψ Relation
by: Brandon S. Hensley
Published: (2025-01-01) -
Red Stellar Populations and Dust Extinction toward W3
by: J. L. Campbell, et al.
Published: (2025-01-01) -
A Catalog of Stellar and Dust Properties for 500,000 Stars in the Southwest Bar of the Small Magellanic Cloud
by: Petia Yanchulova Merica-Jones, et al.
Published: (2025-01-01) -
Uncovering the Hidden Physical Structures and Protostellar Activities in the Low-metallicity S284-RE Region: Results from ALMA and JWST
by: O. R. Jadhav, et al.
Published: (2025-01-01) -
Deep Swift/UVOT Observations of GOODS-N and the Evolution of the Ultraviolet Luminosity Function at 0.2 < z < 1.2
by: Alexander Belles, et al.
Published: (2025-01-01)