120812
2,3-Dimethylindole
≥97%
Sinónimos:
NSC 24936
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About This Item
Fórmula empírica (notación de Hill):
C10H11N
Número de CAS:
Peso molecular:
145.20
EC Number:
MDL number:
UNSPSC Code:
12352100
PubChem Substance ID:
NACRES:
NA.22
Productos recomendados
assay
≥97%
form
solid
bp
285 °C (lit.)
mp
105-107 °C (lit.)
SMILES string
Cc1[nH]c2ccccc2c1C
InChI
1S/C10H11N/c1-7-8(2)11-10-6-4-3-5-9(7)10/h3-6,11H,1-2H3
InChI key
PYFVEIDRTLBMHG-UHFFFAOYSA-N
Application
2,3-Dimethylindole has been used to study the mechanism of oxidation of 2,3-dimethylindole by peroxodisulphate and peroxomonosulphate anions to 2-methylindole-2-carbaldehyde. It has been used to study the behaviour of methylindoles in the agilent multimode ion source by atmospheric pressure chemical ionization mass spectrometry.
Reactant for preparation of:
Reactant for:
- Bis(indolyl)methane derivatives
- Potent opioid receptor agonists
- Photorefractive materials
- Prodrugs of the cyclin-dependent kinase (CDK) inhibitor Alsterpaullone
- Dopamine receptors 2/4 (D2/D4) antagonists
- Useful azaspirocyclic building blocks
Reactant for:
- Baylis-Hillman reactions
- Photosensitized Diels-Alder reactions
- Photoinduced electron transfer reactions
Storage Class
11 - Combustible Solids
wgk_germany
WGK 3
flash_point_f
Not applicable
flash_point_c
Not applicable
ppe
Eyeshields, Gloves, type N95 (US)
Certificados de análisis (COA)
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Direct evidence on the mechanism of the oxidation of 2, 3-dimethylindole by inorganic peroxo anions.
Balon M, et al.
The Journal of Organic Chemistry, 58(26), 7469-7473 (1993)
Formation of the Ions of Methylindoles in APCI Mass Spectrometry.
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ISRN Spectroscopy, 2012 (2012)
A I Novaira et al.
Journal of photochemistry and photobiology. B, Biology, 60(1), 25-31 (2001-06-02)
The quenching of anthracene fluorescence by indole, 1,2-dimethylindole (DMI), tryptophan (Trp) and indole 3-acetic acid (IAA) in palmitoyloleoylphosphatidylcholine (POPC) lipid bilayers was investigated. A very efficient quenching of the anthracene fluorescence in the lipid membrane is observed. Stern-Volmer plots are
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