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...
Príomhchruthaitheoirí: | Gration, A, Magorrian, S |
---|---|
Formáid: | Journal article |
Teanga: | English |
Foilsithe / Cruthaithe: |
Oxford University Press
2024
|
Míreanna comhchosúla
Míreanna comhchosúla
-
Peculiar Dust Emission within the Orion Molecular Cloud
de réir: Parisa Nozari, et al.
Foilsithe / Cruthaithe: (2025-01-01) -
Absence of High-mass Prestellar Cores in the Orion Giant Molecular Cloud
de réir: Wenyu Jiao, et al.
Foilsithe / Cruthaithe: (2024-01-01) -
The Origin of Dust Polarization in the Orion Bar
de réir: Valentin J. M. Le Gouellec, et al.
Foilsithe / Cruthaithe: (2023-01-01) -
Thermodynamics of Giant Molecular Clouds: The Effects of Dust Grain Size
de réir: Nadine H. Soliman, et al.
Foilsithe / Cruthaithe: (2024-01-01) -
Efficacy and safety of inclisiran in patients with cerebrovascular disease: ORION-9, ORION-10, and ORION-11
de réir: Wolfgang Koenig, et al.
Foilsithe / Cruthaithe: (2023-06-01)