It has been thought for many years that the Milky Way is an overly large spiral galaxy. Using Cephied distances to 17 spiral galaxies we calculate the true linear diameters of those galaxies. These diameters are then compared to that of the Milky Way which is found to be, at most, an averagely sized spiral galaxy. When compared to galaxies of approximately the same Hubble type ($2<T<6$) the Milky Way is found to be slightly undersized. This suggests that the Hubble parameter is at the lower end of the currently accepted range of possibilities
The Universe is teeming with galaxies, which are complex structures with a broad range of colors, sh...
We empirically constrain how galaxy size relates to halo virial radius using new measurements of the...
The nature of the spiral structure of the Milky Way has long been debated. Only in the last decade h...
Measurements of the linear diameters of 12 nearby spiral galaxies with distances determined from pri...
International audienceWe compare both the Milky Way and M31 galaxies to local external disk galaxies...
[Abridged]We compare both the Milky Way and M31 galaxies to local external disk galaxies within the ...
International audienceCosmologists have often considered the Milky Way as a typical spiral galaxy, a...
We have produced updated estimates of the scale length of the Milky Way stellar disc by ...
We obtain a robust, non-parametric, estimate of the Hubble constant from galaxy linear diameters cal...
Context. The spiral structure of the Milky Way is not yet well determined. The keys to und...
Recent analyses of Cepheid distances to spiral galaxies have led to the announcement of a Hubble con...
Super spirals are the most massive star-forming disk galaxies in the universe. We measured rotation ...
Master of ScienceDepartment of PhysicsBharat RatraOver three-quarters of observed galaxies are spira...
We present a measurement of the Hubble Constant based on Cepheid distances to 27 galaxies within 20 ...
From our limited perspective—living on a planet that orbits one of several hundred billion stars ins...
The Universe is teeming with galaxies, which are complex structures with a broad range of colors, sh...
We empirically constrain how galaxy size relates to halo virial radius using new measurements of the...
The nature of the spiral structure of the Milky Way has long been debated. Only in the last decade h...
Measurements of the linear diameters of 12 nearby spiral galaxies with distances determined from pri...
International audienceWe compare both the Milky Way and M31 galaxies to local external disk galaxies...
[Abridged]We compare both the Milky Way and M31 galaxies to local external disk galaxies within the ...
International audienceCosmologists have often considered the Milky Way as a typical spiral galaxy, a...
We have produced updated estimates of the scale length of the Milky Way stellar disc by ...
We obtain a robust, non-parametric, estimate of the Hubble constant from galaxy linear diameters cal...
Context. The spiral structure of the Milky Way is not yet well determined. The keys to und...
Recent analyses of Cepheid distances to spiral galaxies have led to the announcement of a Hubble con...
Super spirals are the most massive star-forming disk galaxies in the universe. We measured rotation ...
Master of ScienceDepartment of PhysicsBharat RatraOver three-quarters of observed galaxies are spira...
We present a measurement of the Hubble Constant based on Cepheid distances to 27 galaxies within 20 ...
From our limited perspective—living on a planet that orbits one of several hundred billion stars ins...
The Universe is teeming with galaxies, which are complex structures with a broad range of colors, sh...
We empirically constrain how galaxy size relates to halo virial radius using new measurements of the...
The nature of the spiral structure of the Milky Way has long been debated. Only in the last decade h...