Auriga-California Molecular Cloud Catalog

The Auriga-California molecular cloud is a large region of relatively modest star formation that is part of the Gould Belt. The "Auriga-California Molecular Cloud" (ACMC) Herschel program observed a 14.5 square degree area in five far-infrared bands. The ACMC catalog provides photometry for the 60 point-like and very compact sources in each band: PACS 70 and 160 microns, SPIRE 250, 350, and 500 microns. This dataset or service is made available by the Infrared Science Archive (IRSA) at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

御夫座-加州分子云（Auriga-California Molecular Cloud）是一片恒星形成活动相对平缓的大型天区，隶属于古尔德带（Gould Belt）。御夫座-加州分子云（Auriga-California Molecular Cloud，简称ACMC）赫歇尔观测项目对14.5平方度的天区开展了5个远红外波段的观测。ACMC星表为每个波段内的60个点状致密源提供了测光数据，覆盖波段包括PACS 70微米、160微米，以及SPIRE 250微米、350微米与500微米。本数据集及相关服务由IPAC下属的红外科学档案馆（Infrared Science Archive，简称IRSA）提供，该机构由加州理工学院（California Institute of Technology）按与美国国家航空航天局（National Aeronautics and Space Administration，简称NASA）签订的合同运营。

搜集汇总

背景与挑战

背景概述

Auriga-California分子云目录提供了14.5平方度区域的远红外观测数据，包括PACS和SPIRE五个波段的60个点状和紧凑源的光度测量。该数据集由IPAC发布，旨在支持对Auriga-California分子云的研究。