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090303

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DataCite Commons2024-12-17 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/090303.html
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Dust chemistry is a key tracer of structure formation and evolution. In AGN theorigin and properties of dust are uncertain. Dust could be associated to AGNwinds which would have important implications on the driving and impact of thewinds on their host galaxies. High-resolution X-ray spectroscopy is a novel andpowerful method for probing chemistry of dust. We find NGC 6860 an X-ray brightAGN is an ideal target for investigating the link between dust and winds. Itshows significant reddening and absorption by dust while being sufficientlybright for X-ray spectroscopy. We propose a 120 ks XMM-Newton observation tocarry out high-resolution X-ray spectroscopic study of dust and ionised winds inthis AGN. [truncated! Please see actual data for full text]
提供机构:
European Space Agency
创建时间:
2024-12-17
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