| dc.contributor.author |
O'Brien, DM |
|
| dc.contributor.author |
Ferreira, J |
|
| dc.contributor.author |
Cabrit, S |
|
| dc.contributor.author |
Binette, L |
|
| dc.contributor.author |
García, PJV |
|
| dc.date.accessioned |
2011-01-22T10:26:37Z |
|
| dc.date.available |
2011-01-22T10:26:37Z |
|
| dc.date.issued |
2004 |
|
| dc.identifier.issn |
0004-640X |
|
| dc.identifier.uri |
http://hdl.handle.net/11154/1543 |
|
| dc.description.abstract |
The effects of phenomenological heating functions on the flow thermodynamics of cold T-Tauri disk winds are examined. Turbulent dissipation ( mechanical) heating and a warm disk corona are invoked to heat the wind. The temperature and ionization evolution are solved for along the flow. The results allow the construction of synthetic observations |
en_US |
| dc.description.abstract |
emission maps, forbidden line ratios, line fluxes and line profiles |
en_US |
| dc.description.abstract |
and successfully reproduce a number of observed trends. Mechanical heating produces line ratios and fluxes that fit very well with observations. Invoking a warm disk corona successfully reproduces forbidden line profile low velocity components. |
en_US |
| dc.language.iso |
en |
en_US |
| dc.title |
The temperature and ionization of T-Tauri micro-jets |
en_US |
| dc.type |
Article |
en_US |
| dc.identifier.idprometeo |
1733 |
|
| dc.source.novolpages |
292(40634):609-617 |
|
| dc.subject.wos |
Astronomy & Astrophysics |
|
| dc.description.index |
WoS: SCI, SSCI o AHCI |
|
| dc.subject.keywords |
ISM : jets and outflows |
|
| dc.subject.keywords |
stars : pre-main sequence |
|
| dc.subject.keywords |
MHD |
|
| dc.subject.keywords |
line |
|
| dc.subject.keywords |
profiles |
|
| dc.subject.keywords |
accretion disks |
|
| dc.subject.keywords |
coronae |
|
| dc.relation.journal |
Astrophysics and Space Science |
|