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Materials Data on K(MoS)9 by Materials Project

K(MoS)9 crystallizes in the hexagonal P6_3/m space group. The structure is three-dimensional. K is bonded in a 9-coordinate geometry to nine S atoms. There are three shorter (3.42 Å) and six longer (3.44 Å) K–S bond lengths. There are two inequivalent Mo sites. In the first Mo site, Mo is bonded in a distorted see-saw-like geometry to four S atoms. There are a spread of Mo–S bond distances ranging from 2.49–2.55 Å. In the second Mo site, Mo is bonded in a distorted see-saw-like geometry to four S atoms. There are a spread of Mo–S bond distances ranging from 2.49–2.55 Å. There are two inequivalent S sites. In the first S site, S is bonded in a distorted pentagonal planar geometry to one K and four Mo atoms. In the second S site, S is bonded in a distorted pentagonal planar geometry to one K and four Mo atoms.

36 MATERIALS SCIENCE↗

Materials Data on K(MoS)3 by Materials Project

K(MoS)3 crystallizes in the hexagonal P6_3/m space group. The structure is three-dimensional. K is bonded in a 9-coordinate geometry to nine equivalent S atoms. There are six shorter (3.48 Å) and three longer (3.52 Å) K–S bond lengths. Mo is bonded in a distorted see-saw-like geometry to four equivalent S atoms. There are a spread of Mo–S bond distances ranging from 2.49–2.60 Å. S is bonded in a 7-coordinate geometry to three equivalent K and four equivalent Mo atoms.

36 MATERIALS SCIENCE↗

A 9 month long soft X-ray survey of the Large Magellanic Cloud. I - X-ray map at 1/4 keV

Data from the HEAO 1 low energy detector was used to map the diffuse 1/4 keV X-ray background around the LMC. Data was collected over 9 mos in 1977-1978 using detectors sensitive in the range 0.18-2.8 keV. Diffuse emission, rather than absorption, was observed from the LMC, as were two large emission (2 million K) regions with very low surface brightness. The regions coincided with the Shapley III supergiant shell of optical nebulosity and the LMC bar. Higher spatial resolution imagery is required if the emission features are to be confirmed as the same type of phenomena as the X-ray superbubble in Cygnus.

Singh, K. P.↗