2011
DOI: 10.1007/s12036-011-9020-9
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Chandra Data Analysis of H2O Megamaser Galaxy NGC 4258

Abstract: Chandra observations of NGC 4258 were analyzed to investigate the circumnuclear environment of the H 2 O megamaser galaxy. Its adaptively-smoothed image shows a bright nucleus and another weak source nearby. For the maser host nucleus, our preferred fitting of its spectra gives the absorption of ∼7×10 22 cm −2 .

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“…The disadvantages of universal tool microscope and X-rays are high cost, long cycle and expensive price. Therefore, they are not suitable for the needs of modern industrial development [1][2] .…”
Section: Introductionmentioning
confidence: 99%
“…The disadvantages of universal tool microscope and X-rays are high cost, long cycle and expensive price. Therefore, they are not suitable for the needs of modern industrial development [1][2] .…”
Section: Introductionmentioning
confidence: 99%