Abstract
Luminous ultrasoft NLS1s and low-ionization BALQSOs share many properties, and they both represent important extremes of the active galaxy phenomenon. We briefly discuss their observational similarities as well as potential physical connections between them, concentrating on the X-ray point of view. We present several ways by which potential connections might be further tested.
Original language | English (US) |
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Pages (from-to) | 461-467 |
Number of pages | 7 |
Journal | New Astronomy Reviews |
Volume | 44 |
Issue number | 7-9 |
DOIs | |
State | Published - Sep 2000 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science