International audienceGas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of the protoplanetary disk too cold for the main gas constituent, H2, to emit, alternative tracers such as dust, CO, or the H2 isotopologue HD are used. However, relying on disk mass measurements from any single tracer requires assumptions about the tracer's abundance relative to H2 and the disk temperature structure. Using new Atacama Large Millimeter/submillimeter Array (ALMA) observations from the Molecules with ALMA at Planet-forming Scales (MAPS) ALMA Large Program as well as archival ALMA observations, we construct a disk physical/chemical model of the protoplanetary disk GM Aur. Our model is in good agreement with t...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
Constraining the distribution of gas and dust in the inner 20 au of protoplanetary disks is difficul...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Funding: K.R.S., K.Z., J.B., J.H., and I.C. acknowledge the support of NASA through Hubble Fellowshi...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
Constraining the distribution of gas and dust in the inner 20 au of protoplanetary disks is difficul...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
International audienceGas mass remains one of the most difficult protoplanetary disk properties to c...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Gas mass remains one of the most difficult protoplanetary disk properties to constrain. With much of...
Funding: K.R.S., K.Z., J.B., J.H., and I.C. acknowledge the support of NASA through Hubble Fellowshi...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
International audienceConstraining the distribution of gas and dust in the inner 20 au of protoplane...
Constraining the distribution of gas and dust in the inner 20 au of protoplanetary disks is difficul...