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Time-resolved protoplanetary disk physics in DQ Tau
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创建时间：
2025-02-08
相关数据集
Chandra X-ray Observatory Stack acisfJ1741117m280854_001
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
DataCite Commons2025-02-03 更新30
Chandra X-ray Observatory Stack acisfJ1038583p422813_001
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
DataCite Commons2025-02-03 更新20
Chandra X-ray Observatory Stack acisfJ1737385m283100_001
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
DataCite Commons2025-02-03 更新20
Chandra X-ray Observatory Stack acisfJ0439527p260304_001
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
DataCite Commons2025-02-03 更新30
Chandra X-ray Observatory Stack acisfJ1118304m463411_001
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
DataCite Commons2025-02-03 更新20
