As we continue to investigate and ponder the heavens, we have come to realize the presence of highly energetic gravitational wells at the center of all galaxies. These supermassive black holes at a galaxies nucleus formed in the company of the other features making up the galaxy, particularly spiral arms. With nearby galaxies showing a relationship between the spiral arm pitch angle and that central mass, here we push that relationship out to distances of redshift one. With three galaxies at this distance we find that they also hold to the same relationship of tighter spiral arms corresponding to more massive central black holes. We find that these three galaxies near a redshift of one also fit the equation log M/M⊙ = (8.21 ± 0.16) − (0.062...
Motivated by the evidence of relationships between pitch angle (the tightness of spiral arm structur...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
The past 20 years of observations have revealed correlations between supermassive black holes (SMBHs...
As we continue to investigate and ponder the heavens, we have come to realize the presence of highly...
I extend the empirical correlation between central supermassive black hole mass M and spiral arm pit...
We present Spirality, a novel method of measuring pitch angle by fitting galaxy images to spiral tem...
In this dissertation, I explore the geometric structure of spiral galaxies and how the visible struc...
This dissertation pertains to the geometric structure of late type (spiral) galaxies, specifically o...
Seigar et al. have recently demonstrated a new, tight correlation between galactic central supermass...
Supermassive black holes (SMBHs) are tiny in comparison to the galaxies they inhabit, yet they manag...
We measure the pitch angle ($\varphi$) of spiral arms in a sample of 79 galaxies to perform a system...
In this work, we report a relation between the kinetic energy of random motions of the corresponding...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In an effort to derive accurate bulge magnitudes for the current full sample of 43 spiral galaxies w...
Motivated by the evidence of relationships between pitch angle (the tightness of spiral arm structur...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
The past 20 years of observations have revealed correlations between supermassive black holes (SMBHs...
As we continue to investigate and ponder the heavens, we have come to realize the presence of highly...
I extend the empirical correlation between central supermassive black hole mass M and spiral arm pit...
We present Spirality, a novel method of measuring pitch angle by fitting galaxy images to spiral tem...
In this dissertation, I explore the geometric structure of spiral galaxies and how the visible struc...
This dissertation pertains to the geometric structure of late type (spiral) galaxies, specifically o...
Seigar et al. have recently demonstrated a new, tight correlation between galactic central supermass...
Supermassive black holes (SMBHs) are tiny in comparison to the galaxies they inhabit, yet they manag...
We measure the pitch angle ($\varphi$) of spiral arms in a sample of 79 galaxies to perform a system...
In this work, we report a relation between the kinetic energy of random motions of the corresponding...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In this paper, we study the morphological properties of spiral galaxies, including measurements of s...
In an effort to derive accurate bulge magnitudes for the current full sample of 43 spiral galaxies w...
Motivated by the evidence of relationships between pitch angle (the tightness of spiral arm structur...
Abstract Context.: Spiral galaxies are very common in the local Universe, but their formation, evol...
The past 20 years of observations have revealed correlations between supermassive black holes (SMBHs...