A new model for the luminosity distribution in the inner Milky Way is found, using a non-parametric penalized maximum-likelihood algorithm to deproject a dereddened COBE/ DIRBE L-band map of the inner Galaxy. The model is also constrained by the apparent magnitude (line-of-sight) distributions of clump giant stars in certain bulge fields. An important new feature is the inclusion of a spiral arm model in the disc. Spiral arms make the model appear broader on the sky; thus our bar is more elongated than in previous eight-fold symmetric models. They also lead to a smoother disc model interior to the Sun. The bar length is ≈3.5 kpc, and its axis ratios are 1:(0.3-0.4):0.3, independent of whether the spiral arm model is four-armed or two-armed....
. The color-magnitude diagrams of ¸ 1\Theta10 6 stars obtained for 19 fields towards the Galactic...
We analyze the first-year MACHO collaboration observations of microlensing towards the Galactic cent...
It has been known that recent microlensing results toward the bulge imply mass densities that are su...
A new model for the luminosity distribution in the inner Milky Way is found, using a non-parametric ...
This article summarizes recent work on the luminosity and mass distribution of the Galactic bulge an...
The light distribution in the inner few kiloparsecs of the Milky Way is recovered non- parametricall...
The light distribution in the inner few kiloparsecs of the Milky Way is recovered non-parametrically...
We build a stellar-dynamical model of the Milky Way’s barred bulge and disk, using a newly implement...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Evidence from a variety of sources points towards the existence of a bar in the central few kpc of t...
The microlensing probability (optical depth τ) towards the Galactic Centre carries information about...
. The color-magnitude diagrams of ¸ 1\Theta10 6 stars obtained for 19 fields towards the Galactic...
We analyze the first-year MACHO collaboration observations of microlensing towards the Galactic cent...
It has been known that recent microlensing results toward the bulge imply mass densities that are su...
A new model for the luminosity distribution in the inner Milky Way is found, using a non-parametric ...
This article summarizes recent work on the luminosity and mass distribution of the Galactic bulge an...
The light distribution in the inner few kiloparsecs of the Milky Way is recovered non- parametricall...
The light distribution in the inner few kiloparsecs of the Milky Way is recovered non-parametrically...
We build a stellar-dynamical model of the Milky Way’s barred bulge and disk, using a newly implement...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the...
Evidence from a variety of sources points towards the existence of a bar in the central few kpc of t...
The microlensing probability (optical depth τ) towards the Galactic Centre carries information about...
. The color-magnitude diagrams of ¸ 1\Theta10 6 stars obtained for 19 fields towards the Galactic...
We analyze the first-year MACHO collaboration observations of microlensing towards the Galactic cent...
It has been known that recent microlensing results toward the bulge imply mass densities that are su...