Hogerheijde, M.R.

NARCIS 

Chemical conditions of gas in planet-forming disks

Molecular gas observations of planet-forming disks are undergoing a radical improvement with the sensitivity and resolution of ALMA. Species that until now went undetected can now be imaged, like methanol and other (simple) organics, and rare species like N2D+. At the same time, more 'standard' molecules like CO and its isotopes can be studied at much higher signal-to-noise. Together, these observations are starting to tell us a story of the chemical processes in disks that affect the gas, and on the kinematics inside the disk. I will review recent results, making comparisons to what the dust-continuum observations are showing, and sketch where future observations may take us

Hogerheijde, Michiel

ZENODO

English

<p>Molecular gas observations of planet-forming disks are undergoing a radical improvement with the sensitivity and resolution of ALMA. Species that until now went undetected can now be imaged, like methanol and other (simple) organics, and rare species like N2D+. At the same time, more 'standard' molecules like CO and its isotopes can be studied at much higher signal-to-noise. Together, these observations are starting to tell us a story of the chemical processes in disks that affect the gas, and on the kinematics inside the disk. I will review recent results, making comparisons to what the dust-continuum observations are showing, and sketch where future observations may take us.</p

Hogerheijde, Michiel (5275684)

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Leiden University Scholary Publications

https://figshare.com/articles/Chemical_conditions_of_gas_in_planet-forming_disks/6341290

Chemical conditions of gas in planet-forming disks

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NARCIS

ZENODO

FigShare

Leiden University Scholary Publications