Measuring the Angular Momentum of Supermassive Black Holes (SpringerBriefs in Astronomy)

Measuring The Spin Distribution Of Supermassive Black Holes Is Of Critical Importance For Understanding How These Black Holes And Their Host Galaxies Form And Evolve Over Time, Yet This Type Of Study Is Only In Its Infancy. This Brief Describes How Astronomers Measure Spin In Supermassive Black Holes Using X-ray Spectroscopy. It Also Reviews The Constraints That Have Been Placed On The Spin Distribution In Local, Bright Active Galaxies Over The Past Six Years, And The Cosmological Implications Of These Constraints. Finally, It Summarizes The Open Questions That Remain In This Exciting New Field Of Research And Points Toward Future Discoveries Soon To Be Made By The Next Generation Of Space-based Observatories. I. Introduction On Importance Of Black Hole Spin -- Ii. Description Of Spectroscopic Techniques Used To Measure Spin In Agn -- Iii. Review Of Current Spin Measurements -- Iv. Implications For The Growth Of Black Holes And Their Host Galaxies -- V. Future Directions. By Laura Brenneman. Front Matter....Pages i-v Introduction....Pages 1-4 Measuring Black Hole Spin....Pages 5-9 Applying the Reflection Model....Pages 11-16 Case Studies: MCG–6-30-15, NGC 3783 and Fairall 9....Pages 17-37 Measuring the SMBH Spin Distribution....Pages 39-44 Conclusions and Future Directions....Pages 45-46 Epilogue: NuSTAR Validates Inner Disk Reflection in NGC 1365....Pages 47-49 Back Matter....Pages 51-54