J/A+A/470/605 Halpha and [SII] images in HL/XZ Tau region (Movsessian+, 2007) ================================================================================ Herbig-Haro jets in 3D: the HL/XZ Tauri region. Movsessian T.A., Magakian T.Yu., Bally J., Smith M.D., Moiseev A.V., Dodonov S.N. =2007A&A...470..605M ================================================================================ ADC_Keywords: Interstellar medium Keywords: stars: formation - ISM: jets and outflows - ISM: clouds Description: In this work, we investigated the environment of HL/XZ Tau, which contains a compact and very active nest of YSOs. We explore the kinematic properties of the close association of jets in this region and study the interaction of jets with the ambient medium, as well as the outflows with each other. The scanning Fabry-Perot interferometry of the HL/XZ Tau region in H{alpha} and [SII] 6716{AA} emission lines was performed. We also measure the proper motions of the knots in the outflows, as derived from images obtained in 1997 and 2001, to achieve the full 3D kinematic picture. Objects: ----------------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------------- 04 31 38.5 +18 13 58 HL Tau = 2MASS J04313843+1813576 04 31 40.1 +18 13 57 XZ Tau = 2MASS J04314007+1813571 ----------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file images.dat 53 2 List of images HLTau_Ha.fit 2880 7877 H{alpha} (6555-6568{AA}) 3-D image HLTau_SII.fit 2880 3002 [SII] (6710-6724{AA}) 3-D image -------------------------------------------------------------------------------- Description of file: HLTau_Ha.fts HLTau_SII.fts Common properties of the data cubes stored in the 'fits' subdirectory: * Data are in fits format * Cube axes are: (1) spatial coordinate 1 (2) spatial coordinate 2 (3) wavelength (in Angstroems) * Due to field rotation of 6-m telescope, spatial coordinates do not correspond to equatorial coordinate system. * Heliocentric correction to wavelengths is applied The sizes and spatial sampling of the cubes are not the same because the observations were performed with two different light-acquisition systems. -------------------------------------------------------------------------------- Byte-by-byte Description of file: images.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- FileName Name of the fits file 16- 53 A38 --- Title Title of the file -------------------------------------------------------------------------------- Acknowledgements: Tigran Yu. Magakian, tigmag(at)sci.am ================================================================================ (End) Patricia Vannier [CDS] 04-Aug-2007