2014A&A...567A..13R


Query : 2014A&A...567A..13R

2014A&A...567A..13R - Astronomy and Astrophysics, volume 567A, 13-13 (2014/7-1)

Numerical simulations of stellar jets and comparison between synthetic and observed maps: clues to the launch mechanism.

RUBINI F., MAURRI L., INGHIRAMI G., BACCIOTTI F. and DEL ZANNA L.

Abstract (from CDS):

High angular resolution spectra obtained with the Hubble Space Telescope Imaging Spectrograph (HST/STIS) provide rich morphological and kinematical information about the stellar jet phenomenon, which allows us to test theoretical models efficiently. In this work, numerical simulations of stellar jets in the propagation region are executed with the PLUTO code, by adopting inflow conditions that arise from former numerical simulations of magnetized outflows, accelerated by the disk-wind mechanism in the launching region. By matching the two regions, information about the magneto-centrifugal accelerating mechanism underlying a given astrophysical object can be extrapolated by comparing synthetic and observed position-velocity diagrams. We show that quite different jets, like those from the young T Tauri stars DG-Tau and RW-Aur, may originate from the same disk-wind model for different configurations of the magnetic field at the disk surface. This result supports the idea that all the observed jets may be generated by the same mechanism.

Abstract Copyright:

Journal keyword(s): stars: variables: T Tauri, Herbig Ae/Be - accretion, accretion disks - shock waves - methods: numerical - Herbig-Haro objects

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 HH 702A HH 04 26 35.6281756248 +25 57 53.722465344           ~ 7 0
2 V* DG Tau Or* 04 27 04.6921275888 +26 06 16.060169268 13.57 13.97 10.50 12.28   K6Ve 1024 1
3 V* RW Aur TT* 05 07 49.5662483 +30 24 05.177426   10.86 9.60 9.95   K1/5e+K5e 781 0

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