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Your search keyword '"Thi, W. -F."' showing total 26 results

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26 results on '"Thi, W. -F."'

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1. HCN as a probe of the inner disc in a candidate proto-brown dwarf.

2. First observations of warm and cold methanol in Class 0/I proto-brown dwarfs.

3. survey of HDCO and D2CO towards Class 0/I proto-brown dwarfs.

4. The gas structure of the HD 163296 planet-forming disk - gas gaps or not?

5. The chemistry of episodic accretion

6. First CH3D detection in Class 0/I proto-brown dwarfs: constraints on CH4 abundances.

7. Interpreting high spatial resolution line observations of planet-forming disks with gaps and rings: the case of HD 163296.

8. Warm dust surface chemistry in protoplanetary disks Formation of phyllosilicates.

9. The infrared line-emitting regions of T Tauri protoplanetary disks.

10. The role of atom tunneling in gas-phase reactions in planet-forming disks.

11. Effects of dust evolution on protoplanetary disks in the mid-infrared.

12. Chemical tracers in proto-brown dwarfs: CO, ortho-H2CO, para-H2CO, HCO+, CS observations.

13. Chemical tracers in proto-brown dwarfs: CN, HCN, and HNC observations.

14. Gas lines from the 5-Myr old optically thin disk around HD 141569A

15. The chemistry of episodic accretion in embedded objects 2D radiation thermo-chemical models of the post-burst phase.

16. Thermochemical modelling of brown dwarf discs.

17. The chemistry of episodic accretion.

18. The gas structure of the HD 163296 planet-forming disk - gas gaps or not?

19. Searching for chemical signatures of planet formation.

20. Signatures of warm carbon monoxide in protoplanetary discs observed with Herschel SPIRE★.

21. Observations of Herbig Ae/Be stars with Herschel/PACS The atomic and molecular contents of their protoplanetary discs.

22. Detection of warm water vapour in Taurus protoplanetary discs by Herschel.

23. Gas modelling in the disc of HD 163296.

24. Warm non-equilibrium gas phase chemistry as a possible origin of high HDO/H2O ratios in hot and dense gases: application to inner protoplanetary discs.

25. Continuum and line modelling of discs around young stars – I. 300 000 disc models for HERSCHEL/GASPS.

26. Constraining the stellar energetic particle flux in young solar-like stars.

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