X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
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Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.
X-ray absorption edges indicate diffuse ISM dust towards GX 339-4 consists of Mg-rich amorphous pyroxene (Mg0.75Fe0.25SiO3) and metallic iron.
citing papers explorer
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The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149
X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
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High Resolution X-ray Spectroscopy of the Nova-Like Cataclysmic Variable BZ Cam using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow
Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.
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Dust grain chemistry in the diffuse ISM towards the black hole transient GX 339-4
X-ray absorption edges indicate diffuse ISM dust towards GX 339-4 consists of Mg-rich amorphous pyroxene (Mg0.75Fe0.25SiO3) and metallic iron.