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A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The (vmax, MoM)-( 0, MBH, φ) Relations

The Astrophysical journal, 2019-05, Vol.877 (1), p.64

2019

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Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies

Astrophysical journal. Letters, 2023-10, Vol.956 (1), p.L22

2023

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Efficient Regeneration of Partially Spent Ammonia Borane Fuel

Angewandte Chemie International Edition, 2009-01, Vol.48 (37), p.6812-6816

2009

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STRONG EVIDENCE FOR THE DENSITY-WAVE THEORY OF SPIRAL STRUCTURE IN DISK GALAXIES

Astrophysical journal. Letters, 2016-08, Vol.827 (1), p.L2-L2

2016

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Identification of Intermediate-mass Black Hole Candidates among a Sample of Sd Galaxies

The Astrophysical journal, 2024-08, Vol.971 (2), p.123

2024

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THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES

The Astrophysical journal, 2014-07, Vol.789 (2), p.1-16

2014

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Black Hole Mass Scaling Relations for Early-type Galaxies. I. MBH-M,sph and MBH-M,gal

The Astrophysical journal, 2019-05, Vol.876 (2)

2019

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Black Hole Mass Scaling Relations for Spiral Galaxies. I. MBH-M,sph

The Astrophysical journal, 2019-03, Vol.873 (1)

2019

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Black Hole Mass Scaling Relations for Spiral Galaxies. II. MBH-M,tot and MBH-M,disk

The Astrophysical journal, 2018-12, Vol.869 (2)

2018

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FURTHER EVIDENCE FOR A SUPERMASSIVE BLACK HOLE MASS-PITCH ANGLE RELATION

The Astrophysical journal, 2013-06, Vol.769 (2), p.1-17

2013

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Chemistry of Tris(pentamethylcyclopentadienyl) f-Element Complexes, (C5Me5)3M

Chemical reviews, 2002-06, Vol.102 (6), p.2119-2136

2002

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Calcium Amidotrihydroborate: A Hydrogen Storage Material

Angewandte Chemie (International ed.), 2007-01, Vol.46 (47), p.8995-8997

2007

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Surface-Controlled Conversion of Ammonia Borane from Boron Nitride

Energies (Basel), 2020-10, Vol.13 (21), p.5569

2020

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THE LOCAL BLACK HOLE MASS FUNCTION DERIVED FROM THE MBH-P AND THE MBH-n RELATIONS

The Astrophysical journal, 2016-10, Vol.830 (2)

2016

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Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies

Universe (Basel), 2022-12, Vol.8 (12), p.649

2022

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Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-dependent Substructure in the MBH-nsph and MBH-Re,sph Diagrams: New Tests for Advanced Theories and Realistic Simulations

The Astrophysical journal, 2020-11, Vol.903 (2)

2020

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Spirality: A Novel Way to Measure Spiral Arm Pitch Angle

Galaxies, 2022-10, Vol.10 (5), p.100

2022

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C-H Bond Activation through Steric Crowding of Normally Inert Ligands in the Sterically Crowded Gadolinium and Yttrium (C₅Me₅)₃M Complexes

Proceedings of the National Academy of Sciences - PNAS, 2006-08, Vol.103 (34), p.12678-12683

2006

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Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets

Monthly notices of the Royal Astronomical Society, 2022-06, Vol.514 (3), p.3410-3451

2022

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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, 2021-12, Vol.923 (2), p.246

2021

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Optical and Photophysical Properties of Light-Harvesting Phenylacetylene Monodendrons Based on Unsymmetrical Branching

Journal of the American Chemical Society, 2002-10, Vol.124 (40), p.12002-12012

2002

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Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster

The Astrophysical journal, 2021-12, Vol.923 (2), p.146

2021

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HELLO project: high-z evolution of large and luminous objects

Monthly notices of the Royal Astronomical Society, 2024-08, Vol.533 (2), p.1463-1484

2024

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Impact of Ligand Substitutions on Multielectron Redox Properties of Fe Complexes Supported by Nitrogenous Chelates

ACS omega, 2018-11, Vol.3 (11), p.14766-14778

2018

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Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.512 (1), p.366-377

2022

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A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The (vmax, MoM)-( 0, MBH, φ) Relations

Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies

Efficient Regeneration of Partially Spent Ammonia Borane Fuel

STRONG EVIDENCE FOR THE DENSITY-WAVE THEORY OF SPIRAL STRUCTURE IN DISK GALAXIES

Identification of Intermediate-mass Black Hole Candidates among a Sample of Sd Galaxies

THE BLACK HOLE MASS FUNCTION DERIVED FROM LOCAL SPIRAL GALAXIES

Black Hole Mass Scaling Relations for Early-type Galaxies. I. MBH-M,sph and MBH-M,gal

Black Hole Mass Scaling Relations for Spiral Galaxies. I. MBH-M,sph

Black Hole Mass Scaling Relations for Spiral Galaxies. II. MBH-M,tot and MBH-M,disk

FURTHER EVIDENCE FOR A SUPERMASSIVE BLACK HOLE MASS-PITCH ANGLE RELATION

Chemistry of Tris(pentamethylcyclopentadienyl) f-Element Complexes, (C5Me5)3M

Calcium Amidotrihydroborate: A Hydrogen Storage Material

Surface-Controlled Conversion of Ammonia Borane from Boron Nitride

THE LOCAL BLACK HOLE MASS FUNCTION DERIVED FROM THE MBH-P AND THE MBH-n RELATIONS

Probing the Low-Mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies

Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-dependent Substructure in the MBH-nsph and MBH-Re,sph Diagrams: New Tests for Advanced Theories and Realistic Simulations

Spirality: A Novel Way to Measure Spiral Arm Pitch Angle

C-H Bond Activation through Steric Crowding of Normally Inert Ligands in the Sterically Crowded Gadolinium and Yttrium (C₅Me₅)₃M Complexes

Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets

Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole

Optical and Photophysical Properties of Light-Harvesting Phenylacetylene Monodendrons Based on Unsymmetrical Branching

Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster

HELLO project: high-z evolution of large and luminous objects

Impact of Ligand Substitutions on Multielectron Redox Properties of Fe Complexes Supported by Nitrogenous Chelates

Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters

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