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449431

Sigma-Aldrich

2-Methylindene

98%

Sinonimo/i:

2-Methyl-1H-indene

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About This Item

Formula empirica (notazione di Hill):
C10H10
Numero CAS:
2177-47-1
Peso molecolare:
130.19
Numero MDL:
MFCD00274253
Codice UNSPSC:
12352100
ID PubChem:
24868479
NACRES:
NA.22

Saggio

98%

Indice di rifrazione

n20/D 1.567 (lit.)

P. eboll.

45 °C/0.2 mmHg (lit.)

Densità

0.971 g/mL at 25 °C (lit.)

Stringa SMILE

CC1=Cc2ccccc2C1

InChI

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

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Codice della classe di stoccaggio

10 - Combustible liquids

Classe di pericolosità dell'acqua (WGK)

WGK 3

Punto d’infiammabilità (°F)

168.8 °F - closed cup

Punto d’infiammabilità (°C)

76 °C - closed cup

Certificati d'analisi (COA)

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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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