Calculus
发表于 2025-3-28 18:19:45
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巡回
发表于 2025-3-28 20:00:00
Begriffe, Formen, Regulierungen,regions of normal spiral galaxies, using the near-infrared H and K band CO stellar absorption features. Integral field data from SINFONI will provide high-resolution two-dimensional maps of nuclear velocity dispersion and rotation, which in turn will constrain the anisotropy parameter and yield robust estimates of the central dark mass.
sphincter
发表于 2025-3-29 02:50:29
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绕着哥哥问
发表于 2025-3-29 06:25:31
Graeme K. Deans,Fritz Kröger,Stefan Zeiselct object masses. This is accomplished via optical and IR photometry and spectroscopy of the mass-losing star during the extended X-ray quiescent periods, exploiting essentially classical binary astronomy techniques. I will summarise the optical and IR properties of these objects and review some of the more recent results.
Budget
发表于 2025-3-29 08:17:58
,Dimensionen von Zusammenschlüssen,is above the canonical ., viz., Vela X-1, for which a mass close to . is found. Prospects for progress appear brightest for studies of systems in which the neutron star should have accreted substantial amounts of matter.
察觉
发表于 2025-3-29 15:16:12
https://doi.org/10.1007/978-3-030-99842-45 therefore appears to be a prominent candidate for hosting a black hole in its center. . We demonstrate that with integral field spectroscopy the rotation and velocity dispersion can be much better constrained by sampling in both spatial dimensions. This yields revised and more secure results.
慷慨援助
发表于 2025-3-29 19:35:05
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anticipate
发表于 2025-3-29 22:32:35
Black Holes in X-Ray Binaries,ct object masses. This is accomplished via optical and IR photometry and spectroscopy of the mass-losing star during the extended X-ray quiescent periods, exploiting essentially classical binary astronomy techniques. I will summarise the optical and IR properties of these objects and review some of the more recent results.
Hemiplegia
发表于 2025-3-30 00:11:58
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BALE
发表于 2025-3-30 04:09:32
Effects of Anisotropy on the Central Dark Mass in NGC 3115. New Results from Integral Field Spectro5 therefore appears to be a prominent candidate for hosting a black hole in its center. . We demonstrate that with integral field spectroscopy the rotation and velocity dispersion can be much better constrained by sampling in both spatial dimensions. This yields revised and more secure results.