The Auriga-California molecular cloud is a large region of relatively modest
star formation that is part of the Gould Belt. The Herschel Space Observatory
program OT1_pharvey01_3
("The Auriga-California Molecular Cloud: A Massive Nearby Cloud With Powerful
Diagnostics For Early Stages of Star Formation", PI Paul Harvey) observed a 14.5
square degree area of the cloud in five far-infrared bands. The first delivery
(DR1) of the Herschel program is available here using spatial and visualization
tools.
If you use ACMC data, please cite both the journal article Harvey et al.
(2013) and the dataset Digital Object Identifier (DOI): 10.26131/IRSA23.
Jump to documentation.
|
ACMC Overview
ACMC Primary Data Access
ACMC Catalogs
