AN IMPROVED DYNAMICAL MODEL FOR THE MICROQUASAR XTE J1550–564
We present an improved dynamical model of the X-ray binary and microquasar XTE J1550–564 based on new moderate-resolution optical spectroscopy and near-infrared photometry obtained with the 6.5 m Magellan Telescopes at Las Campanas Observatory. Twelve spectra of the source were obtained using the Ma...
| Päätekijät: | , , , , , , |
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| Muut tekijät: | |
| Aineistotyyppi: | Artikkeli |
| Kieli: | en_US |
| Julkaistu: |
IOP Publishing
2015
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| Linkit: | http://hdl.handle.net/1721.1/95720 |