Weak emission-line quasars (WLQs) are a subset of type 1 quasars that exhibit extremely weak Ly
We examine the UV/X-ray properties of 1378 quasars in order to link empirical correlations to theoretical models of the physical mechanisms dominating quasars as a function of mass and accretion rate. The clarity of these correlations is improved when (1) using C
- Award ID(s):
- 1908716
- NSF-PAR ID:
- 10486233
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 931
- Issue:
- 2
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 154
- Size(s):
- ["Article No. 154"]
- Sponsoring Org:
- National Science Foundation
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