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Plain Text - 91.3 KB - MD5: 6a5fe8b9c679bb78ca1f7ce107bbe045
UBVRI catalog
Lk Ha 101 star forming region
Plain Text - 266.5 KB - MD5: 7e9d2e226d861ef27f8cdb28113902da
UBVRI catalog
NGC 281 star forming region
Plain Text - 804.5 KB - MD5: 6bd4f485ebdfe6775e5f44b3616a18fd
UBVRI catalog
Orion star formign region (not the ONC, but the sourthern extended hockey stick)
Feb 12, 2013
Günther, Hans Moritz, 2012, "Replication data for: Simulating the X-ray emission from accretion shocks on T Tauri stars", https://doi.org/10.7910/DVN/CAQG1T, Harvard Dataverse, V2
Classical T Tauri stars (CTTS) are surrounded by actively accreting disks. According to current models material falls along the magnetic field lines from the disk with more or less free-fall velocity onto the star, where the plasma heats up and generates X-rays. We want to quantitatively explain the observed high energy emission and measure the inf...
Gzip Archive - 1.9 MB - MD5: e33e32df0eca3b8e100253a2ccf6ac3d
Model files
Contains the hydrodynamics for each model. See README for full description.
Gzip Archive - 79.6 MB - MD5: 57dd2331c8cd9d85d45077de2f049666
Model files
Contains the ionization states for each model. See README for full description.
Plain Text - 6.4 KB - MD5: 8b305b8ad328ad4a895aff00dda5697e
README
Describes the file format of all files in this study. Also, shows how to use the fits file to fit your X-ray spectra.
Plain Text - 15.2 MB - MD5: 022c59033719f5bd1c8ae8bdc1d5d873
Model files
This file contains simulated X-ray spectra for the accretion shock on T Tauri stars. Its format and use is explained in the README file.
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