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Davis, Benjamin L., Graham, Alister W., Cameron, Ewan (2019) Black Hole Mass Scaling Relations for Spiral Galaxies. I. M BH–M *,sph. The Astrophysical Journal, 873 (1). 85pp. doi:10.3847/1538-4357/aaf3b8

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Reference TypeJournal (article/letter/editorial)
TitleBlack Hole Mass Scaling Relations for Spiral Galaxies. I. M BH–M *,sph
JournalThe Astrophysical Journal
AuthorsDavis, Benjamin L.Author
Graham, Alister W.Author
Cameron, EwanAuthor
Year2019 (March 6)Volume873
Issue1
PublisherAmerican Astronomical Society
DOIdoi:10.3847/1538-4357/aaf3b8Search in ResearchGate
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Mindat Ref. ID3549487Long-form Identifiermindat:1:5:3549487:0
GUID0
Full ReferenceDavis, Benjamin L., Graham, Alister W., Cameron, Ewan (2019) Black Hole Mass Scaling Relations for Spiral Galaxies. I. M BH–M *,sph. The Astrophysical Journal, 873 (1). 85pp. doi:10.3847/1538-4357/aaf3b8
Plain TextDavis, Benjamin L., Graham, Alister W., Cameron, Ewan (2019) Black Hole Mass Scaling Relations for Spiral Galaxies. I. M BH–M *,sph. The Astrophysical Journal, 873 (1). 85pp. doi:10.3847/1538-4357/aaf3b8
In(2019, March) The Astrophysical Journal Vol. 873 (1) American Astronomical Society

See Also

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Davis, Benjamin L., Graham, Alister W., Cameron, Ewan (2018) Black Hole Mass Scaling Relations for Spiral Galaxies. II. M BH–M *,tot and M BH–M *,disk. The Astrophysical Journal, 869 (2). 113pp. doi:10.3847/1538-4357/aae820
Sahu, Nandini, Graham, Alister W., Davis, Benjamin L. (2019) Black Hole Mass Scaling Relations for Early-type Galaxies. I. M BH–M *, sph and M BH–M *,gal. The Astrophysical Journal, 876 (2). 155pp. doi:10.3847/1538-4357/ab0f32
Davis, Benjamin L., Graham, Alister W., Combes, Françoise (2019) A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The (v max, M oM)–(σ 0, M BH, ϕ) Relations. The Astrophysical Journal, 877 (1). 64pp. doi:10.3847/1538-4357/ab1aa4
Sahu, Nandini, Graham, Alister W., Davis, Benjamin L. (2022) The (Black Hole Mass)–(Spheroid Stellar Density) Relations: M BH–μ (and M BH–Σ) and M BH–ρ. The Astrophysical Journal, 927 (1) 67pp. doi:10.3847/1538-4357/ac4251
Sahu, Nandini, Graham, Alister W., Davis, Benjamin L. (2019) Revealing Hidden Substructures in the M BH–σ Diagram, and Refining the Bend in the L–σ Relation. The Astrophysical Journal, 887 (1). 10pp. doi:10.3847/1538-4357/ab50b7
Graham, Alister W., Scott, Nicholas (2019) Erratum: “The M bh–L spheroid Relation at High and Low Masses, the Quadratic Growth of Black Holes, and Intermediate-mass Black Hole Candidates” (2013, ApJ, 764, 151). The Astrophysical Journal, 874 (1). 110pp. doi:10.3847/1538-4357/ab0e77
Graham, Alister W., Soria, Roberto, Ciambur, Bogdan C., Davis, Benjamin L., Swartz, Douglas A. (2021) Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster. The Astrophysical Journal, 923 (2) 146pp. doi:10.3847/1538-4357/ac235b
Davis, Benjamin L., Graham, Alister W., Soria, Roberto, Jin 金, Zehao 泽灏, Karachentsev, Igor D., Karachentseva, Valentina E., D’Onghia, Elena (2024) Identification of Intermediate-mass Black Hole Candidates among a Sample of Sd Galaxies. The Astrophysical Journal, 971 (2) 123 doi:10.3847/1538-4357/ad55eb
Graham, Alister W., Soria, Roberto, Davis, Benjamin L., Kolehmainen, Mari, Maccarone, Thomas, Miller-Jones, James, Motch, Christian, Swartz, Douglas A. (2021) Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole. The Astrophysical Journal, 923 (2) 246pp. doi:10.3847/1538-4357/ac34f4
Bennert, Vardha N., Treu, Tommaso, Ding, Xuheng, Stomberg, Isak, Birrer, Simon, Snyder, Tomas, Malkan, Matthew A., Stephens, Andrew W., Auger, Matthew W. (2021) A Local Baseline of the Black Hole Mass Scaling Relations for Active Galaxies. IV. Correlations Between M BH and Host Galaxy σ, Stellar Mass, and Luminosity. The Astrophysical Journal, 921 (1) 36pp. doi:10.3847/1538-4357/ac151a
Davis, Benjamin L., Sahu, Nandini, Graham, Alister W. (2020) Substructure in black hole scaling diagrams and implications for the coevolution of black holes and galaxies. Proceedings of the International Astronomical Union, 15. 37-39 doi:10.1017/s1743921320001726
 
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