The Tully-Fisher relationship (TFR) has been shown to have a relatively small observed scatter of ~ +/-0.35 mag implying an intrinsic scatter < +/-0.30 mag. However, when the TFR is calibrated from distances derived from the Hubble relation for field galaxies scatter is consistently found to be +/-0.64 to +/-0.84 mag. This significantly larger scatter requires that intrinsic TFR scatter is actually much larger than +/-0.30 mag, that field galaxies have an intrinsic TFR scatter much larger than cluster spirals, or that field galaxies have a velocity dispersion relative to the Hubble flow in excess of 1000 km s-1. Each of these potential explanations faces difficulties contradicted by available data and the results of previous studies. An alt...
We present an I-band Tully-Fisher relation (TFR) for 18 nearby S0 galaxies using kinematics derived ...
Katherine Kudla ’24 Major: Physics Faculty Mentor: Dr. Joseph Ribaudo, Engineering and Physics The b...
We test and reject the claim of Segal et al. (1993) that the correlation of redshifts and flux densi...
The Tully-Fisher Relationship (TFR) is utilized to identify anomalous redshifts in normal spiral gal...
The statistical properties of the Tully-Fisher relation provide important constraints for semi-analy...
We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Using the Very Large Telescope in Multi Object Spectroscopy mode, we have observed a sample of 113 f...
Local and intermediate redshift galaxy samples obey well correlated relations between the stellar po...
Observational parameters which can be used for redshift-independent distance determination using the...
We present new magnitudes derived from 1.65 mum images for 23 galaxies in the Ursa Major cluster. Ma...
We present the B-band Tully-Fisher relation (TFR) of 60 late-type galaxies with redshifts 0.1-1. The...
The Tully-Fisher (TF) relation is applied to obtain peculiar velocities of field spiral galaxies and...
Context. The study of the evolution of the Tully-Fisher relation has been controversial in the past ...
This thesis presents an exhaustive study of the Tully-Fisher (TF) relation on the basis of the large...
We present an I-band Tully-Fisher relation (TFR) for 18 nearby S0 galaxies using kinematics derived ...
Katherine Kudla ’24 Major: Physics Faculty Mentor: Dr. Joseph Ribaudo, Engineering and Physics The b...
We test and reject the claim of Segal et al. (1993) that the correlation of redshifts and flux densi...
The Tully-Fisher Relationship (TFR) is utilized to identify anomalous redshifts in normal spiral gal...
The statistical properties of the Tully-Fisher relation provide important constraints for semi-analy...
We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] ...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Using the Very Large Telescope in Multi Object Spectroscopy mode, we have observed a sample of 113 f...
Local and intermediate redshift galaxy samples obey well correlated relations between the stellar po...
Observational parameters which can be used for redshift-independent distance determination using the...
We present new magnitudes derived from 1.65 mum images for 23 galaxies in the Ursa Major cluster. Ma...
We present the B-band Tully-Fisher relation (TFR) of 60 late-type galaxies with redshifts 0.1-1. The...
The Tully-Fisher (TF) relation is applied to obtain peculiar velocities of field spiral galaxies and...
Context. The study of the evolution of the Tully-Fisher relation has been controversial in the past ...
This thesis presents an exhaustive study of the Tully-Fisher (TF) relation on the basis of the large...
We present an I-band Tully-Fisher relation (TFR) for 18 nearby S0 galaxies using kinematics derived ...
Katherine Kudla ’24 Major: Physics Faculty Mentor: Dr. Joseph Ribaudo, Engineering and Physics The b...
We test and reject the claim of Segal et al. (1993) that the correlation of redshifts and flux densi...