{"title":"Cover Feature: Deciphering Mg-Surface Interactions with Unsaturated Hydrocarbons: An Integrated Experimental-Theoretical Study (ChemPhysChem 7/2025)","authors":"Sourav Ghoshal, Nathaniel Carnegie, Chidozie Ezeakunne, Beni B. Dangi, Shyam Kattel","doi":"10.1002/cphc.202580702","DOIUrl":null,"url":null,"abstract":"<p><b>The Cover Feature</b> shows polycyclic aromatic hydrocarbons (PAHs), which are essential constituents for forming carbonaceous species in the interstellar medium and on exoplanets. However, the mechanism of the formation of carbonaceous species is not fully understood. In their Research Article (DOI: 10.1002/cphc.202401061), B. B. Dangi, S. Kattel and co-workers provide new insights into the mechanisms of carbonaceous species deposition on magnesium surfaces relevant to exoplanets.\n <figure>\n <div><picture>\n <source></source></picture><p></p>\n </div>\n </figure>\n </p>","PeriodicalId":9819,"journal":{"name":"Chemphyschem","volume":"26 7","pages":""},"PeriodicalIF":2.2000,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1002/cphc.202580702","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chemphyschem","FirstCategoryId":"92","ListUrlMain":"https://chemistry-europe.onlinelibrary.wiley.com/doi/10.1002/cphc.202580702","RegionNum":3,"RegionCategory":"化学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"CHEMISTRY, PHYSICAL","Score":null,"Total":0}
引用次数: 0
Abstract
The Cover Feature shows polycyclic aromatic hydrocarbons (PAHs), which are essential constituents for forming carbonaceous species in the interstellar medium and on exoplanets. However, the mechanism of the formation of carbonaceous species is not fully understood. In their Research Article (DOI: 10.1002/cphc.202401061), B. B. Dangi, S. Kattel and co-workers provide new insights into the mechanisms of carbonaceous species deposition on magnesium surfaces relevant to exoplanets.
覆盖特征显示了多环芳烃（PAHs），这是在星际介质和系外行星上形成碳质物质的必要成分。然而，碳质物质形成的机制尚不完全清楚。在他们的研究论文（DOI: 10.1002/cphc.202401061）中，b.b.。Dangi， S. Kattel及其同事为与系外行星相关的镁表面的碳质物质沉积机制提供了新的见解。
期刊介绍：
ChemPhysChem is one of the leading chemistry/physics interdisciplinary journals (ISI Impact Factor 2018: 3.077) for physical chemistry and chemical physics. It is published on behalf of Chemistry Europe, an association of 16 European chemical societies.
ChemPhysChem is an international source for important primary and critical secondary information across the whole field of physical chemistry and chemical physics. It integrates this wide and flourishing field ranging from Solid State and Soft-Matter Research, Electro- and Photochemistry, Femtochemistry and Nanotechnology, Complex Systems, Single-Molecule Research, Clusters and Colloids, Catalysis and Surface Science, Biophysics and Physical Biochemistry, Atmospheric and Environmental Chemistry, and many more topics. ChemPhysChem is peer-reviewed.
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