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资源简介:
THE X-RAY GAS-TO-DUST ABUNDANCE RATIO OF SILICON TOWARDS GX 17+2
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创建时间:
2023-06-28
相关数据集
Chandra X-ray Observatory Stack acisfJ1600043p413036_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 acisfJ0958281p024145_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
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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



