The Near-ultraviolet Spectra of FU Orionis Accretion Disks
We present the results of the first high-sensitivity near-ultraviolet (NUV; 1800–3200 Å) survey of FU Ori objects, using the Hubble Space Telescope STIS spectrograph. We compare new low-resolution spectra for six sources with predictions from accretion disk models and find that all show emission in...
Tallennettuna:
| Päätekijät: | , , , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2025-01-01
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| Sarja: | The Astrophysical Journal Letters |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/2041-8213/ae1830 |
| Tagit: |
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