Molecular Hydrogen Emission from Protoplanetary Disks

H. Nomura, TJ Millar

Research output: Contribution to journalArticlepeer-review

106 Citations (Scopus)


We have modeled self-consistently the density and temperature profiles of gas and dust in protoplanetary disks, taking into account irradiation from a central star. Making use of this physical structure, we have calculated the level populations of molecular hydrogen and the line emission from the disks. As a result, we can reproduce the observed strong line spectra of molecular hydrogen from protoplanetary disks, both in the ultraviolet (UV) and the near-infrared, but only if the central star has a strong UV excess radiation.
Original languageEnglish
Pages (from-to)923-938
Number of pages16
JournalAstronomy and Astrophysics
Issue number3
Publication statusPublished - Aug 2005

ASJC Scopus subject areas

  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Molecular Hydrogen Emission from Protoplanetary Disks'. Together they form a unique fingerprint.

Cite this