1 / 20

CO Excitation Workshop

CO Excitation Workshop . PDR Benchmark Progress. Starting Point PDR-1 (n=10 3 , =10). Starting Point PDR-2 (n=10 3 , =10 5 ). Starting Point PDR-3 (n=10 5.5 , =10). Starting Point PDR-4 ( n=10 5.5 , =10 5 ). Starting Point PDR-5 ( n=10 7 , =10 ). PDR 4, high n, high FUV.

slade
Download Presentation

CO Excitation Workshop

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. CO Excitation Workshop PDR Benchmark Progress

  2. Starting Point PDR-1 (n=103,=10)

  3. Starting Point PDR-2 (n=103,=105)

  4. Starting Point PDR-3 (n=105.5,=10)

  5. Starting Point PDR-4 (n=105.5,=105)

  6. Starting Point PDR-5 (n=107,=10)

  7. PDR 4, high n, high FUV Tgas n(CO) Large modelscatterlooksscary, but modelassumptionswerevastly different.

  8. Heating/Cooling

  9. Heating/Cooling

  10. PDR 4, high n, high FUV Tgas n(CO) Duringtheworkshopweconcentrate on the „true“ PDR case #4, andtrytounderstandthedifferences

  11. PDR 4, high n, high FUV NEW Tgas n(CO) Duringtheworkshopweconcentrate on the „true“ PDR case #4, andtrytounderstandthedifferences

  12. PDR 4, high n, high FUV PE Heating, H2formationheating Dustcontent NEW Tgas n(CO) Duringtheworkshopweconcentrate on the „true“ PDR case #4, andtrytounderstandthedifferences

  13. Starting Point PDR-4 (n=105.5,=105)

  14. Starting Point PDR-4 (n=105.5,=105) NEW

  15. Additional Information

  16. Additional Information • Dusttemperaturesappearconsistent • Temperaturerangeforgrainsizedistributionscomparable • Relativelyhotdustthroughoutthewholecloud!

  17. Additional Information • Major heatingthroughphoto-electricheating • NO PAHs ! • Differencesremain(FUV field?, electrondensity, …)

  18. Additional Information Major coolants [OI] gas-graincollisison

  19. Additional Information Major coolants [OI] gas-graincollisison

  20. Summary • Giventhecomplexity of thevariouscodesandthevagueness of thebenchmark (round 2) specificstheconvergence of theresultsis still remarkable. • Nonewmajorheating/coolingprocesscandidate • Major processesare : • Dustphysics • H2formation • FUV?? • But theirdetailsremaintobeinvestigated

More Related