Measurements of the linear diameters of 12 nearby spiral galaxies with distances determined from primary indicators suggest that both the Milky Way Galaxy and M31 are in the middle of the range of sizes for such galaxies. By comparing the measured linear diameters of these nearby systems with the inferred diameters of a sample of more than 3000 spirals with known redshifts, we conclude that the most likely value of the Hubble Parameter lies in the range 50 - 55 km/s Mpc^{-1}
In this paper we derive a Tully Fisher relation from measured I band photometry and H\alpha rotation...
Significant progress has been made during the last 10 years toward resolving the debate over the exp...
International audienceWe compare both the Milky Way and M31 galaxies to local external disk galaxies...
It has been thought for many years that the Milky Way is an overly large spiral galaxy. Using Cephie...
We obtain a robust, non-parametric, estimate of the Hubble constant from galaxy linear diameters cal...
Recent analyses of Cepheid distances to spiral galaxies have led to the announcement of a Hubble con...
The three rung distance ladder, which calibrates Type Ia supernovae through stellar distances linked...
Abstract. The value of Hubble parameter (H0) is determined using the morphologically type dependent ...
We present a measurement of the Hubble Constant based on Cepheid distances to 27 galaxies within 20 ...
New Hubble Space Telescope observations of Cepheid variable stars in the nearby galaxy M96 give a di...
We empirically constrain how galaxy size relates to halo virial radius using new measurements of the...
The importance of the distance of the Virgo cluster in the ongoing debate on the value of the Hubble...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
Water megamasers residing in the accretion disks around supermassive black holes (SMBHs) in active g...
This thesis presents an exhaustive study of the Tully-Fisher (TF) relation on the basis of the large...
In this paper we derive a Tully Fisher relation from measured I band photometry and H\alpha rotation...
Significant progress has been made during the last 10 years toward resolving the debate over the exp...
International audienceWe compare both the Milky Way and M31 galaxies to local external disk galaxies...
It has been thought for many years that the Milky Way is an overly large spiral galaxy. Using Cephie...
We obtain a robust, non-parametric, estimate of the Hubble constant from galaxy linear diameters cal...
Recent analyses of Cepheid distances to spiral galaxies have led to the announcement of a Hubble con...
The three rung distance ladder, which calibrates Type Ia supernovae through stellar distances linked...
Abstract. The value of Hubble parameter (H0) is determined using the morphologically type dependent ...
We present a measurement of the Hubble Constant based on Cepheid distances to 27 galaxies within 20 ...
New Hubble Space Telescope observations of Cepheid variable stars in the nearby galaxy M96 give a di...
We empirically constrain how galaxy size relates to halo virial radius using new measurements of the...
The importance of the distance of the Virgo cluster in the ongoing debate on the value of the Hubble...
Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher r...
Water megamasers residing in the accretion disks around supermassive black holes (SMBHs) in active g...
This thesis presents an exhaustive study of the Tully-Fisher (TF) relation on the basis of the large...
In this paper we derive a Tully Fisher relation from measured I band photometry and H\alpha rotation...
Significant progress has been made during the last 10 years toward resolving the debate over the exp...
International audienceWe compare both the Milky Way and M31 galaxies to local external disk galaxies...