Abstract
I began this thesis with the statement that accreting systems and their associated outflows are astrophysically important.
...and the credits rave as the critics roll.
Mike Vennart, Silent/Transparent
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Arav N, Becker RH, Laurent-Muehleisen SA, Gregg MD, White RL, Brotherton MS, de Kool M (1999a) What Determines the Depth of Broad Absorption Lines? Keck HIRES Observations of BALQSO 1603+3002. ApJ 524:566–571. doi:10.1086/307841. arXiv:astro-ph/9903140
Arav N, Korista KT, de Kool M, Junkkarinen VT, Begelman MC (1999b) Hubble Space Telescope Observations of the Broad Absorption Line QuasarPG 0946+301. ApJ 516:27–46. doi:10.1086/307073. arXiv:astro-ph/9810309
Dai X, Shankar F, Sivakoff GR (2012) The Intrinsic Fractions and Radio Properties of Low-ionization Broad Absorption Line Quasars. ApJ 757:180. doi:10.1088/0004-637X/757/2/180. arXiv:1004.0700
de Kool M, Begelman MC (1995) Radiation Pressure-driven Magnetic Disk Winds in Broad Absorption Line Quasi-stellar Objects. ApJ 455:448. doi:10.1086/176594
Edelson R, Gelbord JM, Horne K, McHardy IM, Peterson BM, Arévalo P, Breeveld AA, De Rosa G, Evans PA, Goad MR, Kriss GA, Brandt WN, Gehrels N, Grupe D, Kennea JA, Kochanek CS, Nousek JA, Papadakis I, Siegel M, Starkey D, Uttley P, Vaughan S, Young S, Barth AJ, Bentz MC, Brewer BJ, Crenshaw DM, Dalla Bontà E, De Lorenzo-Cáceres A, Denney KD, Dietrich M, Ely J, Fausnaugh MM, Grier CJ, Hall PB, Kaastra J, Kelly BC, Korista KT, Lira P, Mathur S, Netzer H, Pancoast A, Pei L, Pogge RW, Schimoia JS, Treu T, Vestergaard M, Villforth C, Yan H, Zu Y (2015) Space Telescope and Optical Reverberation Mapping Project. II. Swift and HST Reverberation Mapping of the Accretion Disk of NGC 5548. ApJ 806:129. doi:10.1088/0004-637X/806/1/129. arXiv:1501.05951
Elvis M (2000) A Structure for Quasars. ApJ 545:63–76. doi:10.1086/317778. arXiv:astro-ph/0008064
Gaetz TJ, Salpeter EE (1983) Line radiation from a hot, optically thin plasma - Collision strengths and emissivities. ApJs 52:155–168. doi:10.1086/190862
Hamann WR, Oskinova LM, Feldmeier A (2008) Spectrum formation in clumpy stellar winds. In: Hamann WR, Feldmeier A, Oskinova LM (eds) Clumping in Hot-Star Winds, p 75
Horne K, Marsh TR, Cheng FH, Hubeny I, Lanz T (1994) HST eclipse mapping of dwarf nova OY Carinae in quiescence: an ’Fe II curtain’ with Mach approx. = 6 velocity dispersion veils the white dwarf. ApJ 426:294–307. doi:10.1086/174064
Lucy LB (2002) Monte Carlo transition probabilities. A&A384:725–735. doi:10.1051/0004-6361:20011756. arXiv:astro-ph/0107377
Lucy LB (2003) Monte Carlo transition probabilities. II. A&A403:261–275. doi:10.1051/0004-6361:20030357. arXiv:astro-ph/0303202
Marsh TR, Horne K (1988) Images of accretion discs. II - Doppler tomography. MNRAS 235:269–286. doi:10.1093/mnras/235.1.269
Muñoz-Darias T, Casares J, Mata Sánchez D, Fender RP, Armas Padilla M, Linares M, Ponti G, Charles PA, Mooley KP, Rodriguez J (2016) Regulation of black-hole accretion by a disk wind during a violent outburst of V404 Cygni. Nature. doi:10.1038/nature17446. arXiv:astro-ph/0312379
Netzer H (1990) AGN emission lines. In: Blandford RD, Netzer H, Woltjer L, Courvoisier TJL, Mayor M (eds) Active Galactic Nuclei, pp 57–160
Noebauer UM, Long KS, Sim SA, Knigge C (2010) The Geometry and Ionization Structure of the Wind in the Eclipsing Nova-like Variables RW Tri and UX UMa. ApJ 719:1932–1945. doi:10.1088/0004-637X/719/2/1932. arXiv:1007.0209
Risaliti G, Salvati M, Marconi A (2011) [O III] equivalent width and orientation effects in quasars. MNRAS 411:2223–2229. doi:10.1111/j.1365-2966.2010.17843.x. arXiv:1010.2037
Shen Y, Ho LC (2014) The diversity of quasars unified by accretion and orientation. Nature 513:210–213. doi:10.1038/nature13712. arXiv:1409.2887
Stalevski M, Fritz J, Baes M, Popovic LC (2013) The AGN dusty torus as a clumpy two-phase medium: radiative transfer modeling with SKIRT. ArXiv e-prints arXiv:1301.4244
Šurlan B, Hamann WR, Kubát J, Oskinova LM, Feldmeier A (2012) Three-dimensional radiative transfer in clumped hot star winds. I. Influence of clumping on the resonance line formation. A&A 541:A37. doi:10.1051/0004-6361/201118590. arXiv:1202.4787
Urrutia T, Becker RH, White RL, Glikman E, Lacy M, Hodge J, Gregg MD (2009) The FIRST-2MASS Red Quasar Survey. II. An Anomalously High Fraction of LoBALs in Searches for Dust-Reddened Quasars. ApJ 698:1095–1109. doi:10.1088/0004-637X/698/2/1095. arXiv:0808.3668
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2017 Springer International Publishing AG
About this chapter
Cite this chapter
Matthews, J. (2017). Conclusions and Future Work. In: Disc Winds Matter. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-59183-4_7
Download citation
DOI: https://doi.org/10.1007/978-3-319-59183-4_7
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-59182-7
Online ISBN: 978-3-319-59183-4
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)