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29162-92-3

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29162-92-3 Usage

Check Digit Verification of cas no

The CAS Registry Mumber 29162-92-3 includes 8 digits separated into 3 groups by hyphens. The first part of the number,starting from the left, has 5 digits, 2,9,1,6 and 2 respectively; the second part has 2 digits, 9 and 2 respectively.
Calculate Digit Verification of CAS Registry Number 29162-92:
(7*2)+(6*9)+(5*1)+(4*6)+(3*2)+(2*9)+(1*2)=123
123 % 10 = 3
So 29162-92-3 is a valid CAS Registry Number.

29162-92-3SDS

SAFETY DATA SHEETS

According to Globally Harmonized System of Classification and Labelling of Chemicals (GHS) - Sixth revised edition

Version: 1.0

Creation Date: Aug 18, 2017

Revision Date: Aug 18, 2017

1.Identification

1.1 GHS Product identifier

Product name 2-iodo-1,3-dimethyl-1,3-diaza-2-borinane

1.2 Other means of identification

Product number -
Other names 2-Jod-1,3-dimethyl-1,3-diaza-2-borinan

1.3 Recommended use of the chemical and restrictions on use

Identified uses For industry use only.
Uses advised against no data available

1.4 Supplier's details

1.5 Emergency phone number

Emergency phone number -
Service hours Monday to Friday, 9am-5pm (Standard time zone: UTC/GMT +8 hours).

More Details:29162-92-3 SDS

29162-92-3Downstream Products

29162-92-3Relevant articles and documents

Boron-nitrogen compounds. XXXIV. Preparation and some properties of 2-halo-1,3,2-diazaboracycloalkanes

Wang, Tai-Tzer,Busse, Paul J.,Niedenzu, Kurt

, p. 2150 - 2152 (2008/10/08)

A series of 2-halo-1,3,2-diazaboracycloalkanes has been prepared by (a) the interaction of trialkylamine-trihaloboranes with alphatic α,ω-diamines, (b) displacement of dimethylamino groups of 2-dimethylamino-1,3,2-diazaboracycloalkanes with halogen through interaction with boron trihalides, and (c) a transhalogenation reaction. The 2-halo-1,3,2-diazaboracycloalkanes are thermally rather stable but are very reactive toward moisture and oxygen. The boron-bonded halogen is readily replaced by organic groups through interaction with Grignard reagents. All compounds have a characteristic BN absorption in the 1510-1540-cm-1 region of their infrared spectra and the proton magnetic resonance spectra are consistent with their structure. In the mass spectra, the parent peaks P+ are generally less abundant than the (P - 1)+ peaks.

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