Mapping dust in the giant molecular cloud Orion A
The Sun is located close to the Galactic mid-plane, meaning that we observe the Galaxy through significant quantities of dust. Moreover, the vast majority of the Galaxy’s stars also lie in the disc, meaning that dust has an enormous impact on the massive astrometric, photometric and spectroscopic su...
المؤلفون الرئيسيون: | Gration, A, Magorrian, S |
---|---|
التنسيق: | Journal article |
اللغة: | English |
منشور في: |
Oxford University Press
2024
|
مواد مشابهة
-
Peculiar Dust Emission within the Orion Molecular Cloud
حسب: Parisa Nozari, وآخرون
منشور في: (2025-01-01) -
Absence of High-mass Prestellar Cores in the Orion Giant Molecular Cloud
حسب: Wenyu Jiao, وآخرون
منشور في: (2024-01-01) -
The Origin of Dust Polarization in the Orion Bar
حسب: Valentin J. M. Le Gouellec, وآخرون
منشور في: (2023-01-01) -
Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size
حسب: Nadine H. Soliman, وآخرون
منشور في: (2024-01-01) -
Efficacy and safety of inclisiran in patients with cerebrovascular disease: ORION-9, ORION-10, and ORION-11
حسب: Wolfgang Koenig, وآخرون
منشور في: (2023-06-01)