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About This Item
Empirical Formula (Hill Notation):
Kr
CAS Number:
Molecular Weight:
83.80
EC Number:
MDL number:
UNSPSC Code:
12352300
PubChem Substance ID:
NACRES:
NA.23
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Assay
≥99.998%
SMILES string
[Kr]
InChI
1S/Kr
InChI key
DNNSSWSSYDEUBZ-UHFFFAOYSA-N
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Packaging
pressure tin
filling pressure at 15°C: 11 bar; content (15°C, 1 bar): 11 l
filling pressure at 15°C: 11 bar; content (15°C, 1 bar): 11 l
Other Notes
Sales restrictions may apply
Signal Word
Warning
Hazard Statements
Precautionary Statements
Hazard Classifications
Press. Gas Compr. Gas
Storage Class Code
2A - Gases
WGK
nwg
Flash Point(F)
Not applicable
Flash Point(C)
Not applicable
Personal Protective Equipment
dust mask type N95 (US), Eyeshields, Gloves
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Dieter Hauchecorne et al.
Physical chemistry chemical physics : PCCP, 13(21), 10204-10213 (2011-04-22)
Using FTIR and Raman spectroscopy, the formation of halogen bonded complexes of the trifluorohalomethanes CF(3)Cl, CF(3)Br and CF(3)I with dimethyl sulfide (DMS) dissolved in liquid krypton has been investigated. For CF(3)Br and CF(3)I, evidence was found for the formation of
Carlos A Fernandez et al.
Journal of the American Chemical Society, 134(22), 9046-9049 (2012-05-18)
Krypton (Kr) and xenon (Xe) adsorption on two partially fluorinated metal-organic frameworks (FMOFCu and FMOFZn) with different cavity size and topologies are reported. FMOFCu shows an inversion in sorption selectivity toward Kr at temperatures below 0 °C while FMOFZn does
Anne-Lise Hachulla et al.
Radiology, 263(1), 253-259 (2012-02-15)
To evaluate the tolerance and level of enhancement achievable after inhalation of stable krypton. This study was approved by the institutional review board and the local ethics committee. Written informed consent was obtained from all subjects. The study was planned
Joseph S Six et al.
PloS one, 7(11), e49927-e49927 (2012-12-05)
Hyperpolarized (hp) (129)Xe and hp (83)Kr for magnetic resonance imaging (MRI) are typically obtained through spin-exchange optical pumping (SEOP) in gas mixtures with dilute concentrations of the respective noble gas. The usage of dilute noble gases mixtures requires cryogenic gas
Lu Zhang et al.
Optics express, 19(25), 25812-25822 (2012-01-26)
We observed that increasing the clusters size and laser pulse contrast can enhance the X-ray flux emitted by femtosecond-laser-driven-cluster plasma. By focusing a high contrast laser (10(-10)) on large argon clusters, high flux Kα-like X-rays (around 2.96 keV) is generated
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