Get Quote

((Isopropoxymethoxy)methoxy)methanol (CAS 100208-42-2)

((Isopropoxymethoxy)methoxy)methanol (CAS: 100208-42-2) has molecular formula C6H14O4 and molecular weight 150.17 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 ((Isopropoxymethoxy)methoxy)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

Detailed Literature Analysis

Below are the top-ranked research papers for ((Isopropoxymethoxy)methoxy)methanol, presented with bibliographic details and scientific abstracts.

Synthetic Chemistry

1. Level alignment of a prototypical photocatalytic system: Methanol on TiO2(110)
Annapaola Migani, Duncan J. Mowbray, Amilcare Iacomino, Jin Zhao, Hrvoje Petek; arXiv preprint
Photocatalytic and photovoltaic activity depends on the optimal alignment of electronic levels at the molecule/semiconductor interface. Establishing level alignment experimentally is complicated by the uncertain chemical identity of the surface species. We address the assignment of the occupied and empty electronic levels for the prototypical photo
2. Level alignment of a prototypical photocatalytic system: Methanol on TiO2(110)
Annapaola Migani, Duncan J. Mowbray, Amilcare Iacomino, Jin Zhao, Hrvoje Petek; arXiv preprint
Photocatalytic and photovoltaic activity depends on the optimal alignment of electronic levels at the molecule/semiconductor interface. Establishing level alignment experimentally is complicated by the uncertain chemical identity of the surface species. We address the assignment of the occupied and empty electronic levels for the prototypical photo
3. The role of surface defects in the adsorption of methanol on Fe3O4(001)
Oscar Gamba, Jan Hulva, Jiri Pavelec, Roland Bliem, Michael Schmid; arXiv preprint
The adsorption of methanol (CH3OH) at the Fe3O4(001)-c(2x2) surface was studied using X-ray photoelectron spectroscopy (XPS), scanning tunneling microscopy (STM), and temperature-programmed desorption (TPD). CH3OH adsorbs exclusively at surface defects sites at room temperature to form hydroxyl groups and methoxy (CH3O) species. Active sites are id
4. The role of surface defects in the adsorption of methanol on Fe3O4(001)
Oscar Gamba, Jan Hulva, Jiri Pavelec, Roland Bliem, Michael Schmid; arXiv preprint
The adsorption of methanol (CH3OH) at the Fe3O4(001)-c(2x2) surface was studied using X-ray photoelectron spectroscopy (XPS), scanning tunneling microscopy (STM), and temperature-programmed desorption (TPD). CH3OH adsorbs exclusively at surface defects sites at room temperature to form hydroxyl groups and methoxy (CH3O) species. Active sites are id

Other Research

5. The Methanol Multibeam Survey
J. A. Green, the Methanol Multibeam Survey Collaboration; arXiv preprint
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
6. The Methanol Multibeam Survey
J. A. Green, the Methanol Multibeam Survey Collaboration; arXiv preprint
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
7. Detection of a 6.7 GHz methanol kilomaser toward NGC4945
Simon Ellingsen, Tiege McCarty, Shari Breen, Maxim Voronkov; arXiv preprint
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
8. Detection of a 6.7 GHz methanol kilomaser toward NGC4945
Simon Ellingsen, Tiege McCarty, Shari Breen, Maxim Voronkov; arXiv preprint
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

Conclusion

The research literature on ((Isopropoxymethoxy)methoxy)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. 8 papers analyzed. Last updated: 2026-05-25. This article is automatically generated from peer-reviewed research data.