C. Jager

collaborators

3 papers

astro-ph.EP2025

Evidence for SiO cloud nucleation in the rogue planet PSO J318

P. MolliÃ¨re, H. KÃ¼hnle, E. C. Matthews +25

Silicate clouds are known to significantly impact the spectra of late L-type brown dwarfs, with observable absorption features at ~ 10 micron. JWST has reopened our window to the m…

astro-ph.GA2024

Infrared Spectra of Solid-State Ethanolamine: Laboratory Data in Support of JWST Observations

T. Suhasaria, S. M. Wee, R. BasalgÃ¨te +4

Ethanolamine (NH $_{2}$ CH $_{2}$ CH $_{2}$ OH, EA) has been identified in the gas phase of the ISM within molecular clouds. Although EA has not been directly observed in the molecular ice pha…

astro-ph.GA2024

Formation of N-bearing complex organic molecules in molecular clouds: Ketenimine, acetonitrile, acetaldimine, and vinylamine via the UV photolysis of C $_{2}$ H $_{2}$ ice

K. -J. Chuang, C. JÃ¤ger, J. C. Santos +1

The solid-state C $_{2}$ H $_{2}$ chemistry in interstellar H $_{2}$ O-rich ice has been proposed to explain astronomically observed complex organic molecules (COMs), including ketene (CH $_{2}$ …

Evidence for SiO cloud nucleation in the rogue planet PSO J318

Infrared Spectra of Solid-State Ethanolamine: Laboratory Data in Support of JWST Observations

Formation of N-bearing complex organic molecules in molecular clouds: Ketenimine, acetonitrile, acetaldimine, and vinylamine via the UV photolysis of C2​H2​ ice

Formation of N-bearing complex organic molecules in molecular clouds: Ketenimine, acetonitrile, acetaldimine, and vinylamine via the UV photolysis of C $_{2}$ H $_{2}$ ice