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449431

Sigma-Aldrich

2-Methylindene

98%

Synonym(s):

2-Methyl-1H-indene

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About This Item

Empirical Formula (Hill Notation):
C10H10
CAS Number:
2177-47-1
Molecular Weight:
130.19
MDL number:
MFCD00274253
UNSPSC Code:
12352100
PubChem Substance ID:
24868479
NACRES:
NA.22

Assay

98%

refractive index

n20/D 1.567 (lit.)

bp

45 °C/0.2 mmHg (lit.)

density

0.971 g/mL at 25 °C (lit.)

SMILES string

CC1=Cc2ccccc2C1

InChI

1S/C10H10/c1-8-6-9-4-2-3-5-10(9)7-8/h2-6H,7H2,1H3

InChI key

YSAXEHWHSLANOM-UHFFFAOYSA-N

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Storage Class Code

10 - Combustible liquids

WGK

WGK 3

Flash Point(F)

168.8 °F - closed cup

Flash Point(C)

76 °C - closed cup

Certificates of Analysis (COA)

Search for Certificates of Analysis (COA) by entering the products Lot/Batch Number. Lot and Batch Numbers can be found on a product’s label following the words ‘Lot’ or ‘Batch’.

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I Ogawa et al.
Talanta, 28(10), 725-729 (1981-10-01)
The degradation of acenaphthylene, acenaphthene, 2-methylnaphthalene, 2-methylindene, 3-methylindene and indene in water solutions was studied. These compounds at the 25-150 mug/l. level were almost totally degraded at ambient temperature within three days. The microbial population responsible for the degradation occurs
Antimicrobial effect of monomers and polymers with azole moieties.
Moon W-S, et al.
Journal of Applied Polymer Science, 90(11), 2933-2937 (2003)
Mike McD Francis et al.
Canadian journal of microbiology, 49(11), 699-706 (2004-01-22)
A purified microbial isolate, identified as a strain of Rhodococcus sp., metabolized indene primarily to iso quinoline and lesser amounts of indandiol and indanone. Isoquinoline production was dependent on the presence of microbial culture, indene, and ammonium ions as the
Decomposition, isomerization, and ring expansion in 2-methylindene: Single-pulse shock tube and modeling study.
Lifshitz A, et al.
The Journal of Physical Chemistry A, 108(16), 3430-3438 (2004)
Long Zhao et al.
Nature communications, 10(1), 3689-3689 (2019-08-17)
Polycyclic aromatic hydrocarbons (PAHs) represent key molecular building blocks leading to carbonaceous nanoparticles identified in combustion systems and extraterrestrial environments. However, the understanding of their formation and growth in these high temperature environments has remained elusive. We present a mechanism

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