(1-Aminocyclopentyl)methanol (CAS 10316-79-7)
(1-Aminocyclopentyl)methanol (CAS:
10316-79-7) has molecular formula C6H13NO and molecular weight 115.17 g/mol. This compound has been the subject of numerous scientific investigations due to its structural features and practical utility in synthetic chemistry and industrial processes. View product details →
Product Background
This comprehensive research profile examines the scientific literature surrounding (1-Aminocyclopentyl)methanol.
Key Research Findings
- I will discuss the techniques and properties of the MMB survey, before outlining recent results, which include the identification of regions of enhanced star formation believed to
- We employ the well-tested vdW-DF method that seamlessly includes dispersion interactions with all of the more close-ranged interactions that result in bonds like the covalent and h
- We report the results of a search for class II methanol masers at 37.7, 38.3 and 38.5 GHz towards a sample of 70 high-mass star formation regions.
Detailed Literature Analysis
Below are the top-ranked research papers for (1-Aminocyclopentyl)methanol, presented with bibliographic details and scientific abstracts.
Biological & Pharmacological Studies
1. 37 GHz methanol masers : Horsemen of the Apocalypse for the class II methanol maser phase?
We report the results of a search for class II methanol masers at 37.7, 38.3 and 38.5 GHz towards a sample of 70 high-mass star formation regions. We primarily searched towards regions known to show emission either from the 107 GHz class II methanol maser transition, or from the 6.035 GHz excited OH transition. We detected maser emission from 13 so
🔑 Key Finding: We report the results of a search for class II methanol masers at 37.7, 38.3 and 38.5 GHz towards a sample of 70 high-mass star formation regions.
Other Research
2. The Methanol Multibeam Survey
A purpose built 7-beam methanol receiver, installed on the Parkes Radio Telescope, was used to survey the Galactic plane for newly forming high mass stars, pinpointed by strong methanol maser emission at 6.7 GHz. The Methanol Multibeam (MMB) survey observed over 60% of the Galactic plane, detecting close to 1000 sources. The MMB survey provides a h
3. Detection of a 6.7 GHz methanol kilomaser toward NGC4945
We report the detection of emission from the 6.7 GHz 5(1)-6(0)A+ transition of methanol towards the center of the nearby galaxy NGC4945. This is the first detection of emission in this transition beyond the local group. The isotropic luminosity of the integrated 6.7 GHz methanol emission is approximately a factor of 10000 greater than that for 6.7
4. Methanol adsorption on graphene
The adsorption energies and orientation of methanol on graphene are determined from first-principles density functional calculations. We employ the well-tested vdW-DF method that seamlessly includes dispersion interactions with all of the more close-ranged interactions that result in bonds like the covalent and hydrogen bonds. The adsorption of a s
5. Methanol in the L1551 Circumbinary Torus
We report observations of gaseous methanol in an edge-on torus surrounding the young stellar object L1551 IRS5. The peaks in the torus are separated by ~ 10,000 AU from L1551 IRS5, and contain ~ 0.03 earth masses of cold methanol. We infer that the methanol abundance increases in the outer part of the torus, probably as a result of methanol evapora
Conclusion
The research literature on (1-Aminocyclopentyl)methanol demonstrates sustained scientific interest, with publications continuing through 0. The compound serves as an important building block in synthetic chemistry and has been explored for various applications. Researchers and industrial users can view detailed specifications or submit an inquiry for pricing and availability.
Data Sources: PubMed/MEDLINE, CrossRef. 5 papers analyzed. Last updated: 2026-05-25. This article is automatically generated from peer-reviewed research data.