Recent mass estimates for Milky and the Local Group

In summary, the authors of this study used the Millennium Simulation to calibrate the bias and error distribution of Timing Argument estimators for estimating the masses of the Local Group and the Milky Way. Using this method, they found that the interquartile range of the ratio of timing mass to true mass was a factor of 1.8, with a 5% to 95% range of a factor of 5.7. This led to an estimated median likelihood of the true mass of the Local Group as 5.27 x 10^12 solar masses, with a 95% lower confidence limit of 1.81 x 10^12 solar masses. They also estimated the virial mass of the Milky Way to
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http://arxiv.org/abs/0710.3740
Masses for the Local Group and the Milky Way
Yang-Shyang Li (1), Simon D. M. White (2) ((1) Kapteyn Astronomical Institute, (2) Max-Plank-Institut für Astrophysik)
10 pages, 5 figures, Submitted to MNRAS
(Submitted on 19 Oct 2007)

"We use the very large Millennium Simulation of the concordance LambdaCDM cosmogony to calibrate the bias and error distribution of Timing Argument estimators of the masses of the Local Group and of the Milky Way. From a large number of isolated spiral-spiral pairs similar to the Milky Way/Andromeda system, we find the interquartile range of the ratio of timing mass to true mass to be a factor of 1.8, while the 5% and 95% points of the distribution of this ratio are separated by a factor of 5.7. Here we define true mass as the sum of the 'virial' masses [tex]M_{200}[/tex] of the two dominant galaxies. For current best values of the distance and approach velocity of Andromeda this leads to a median likelihood estimate of the true mass of the Local Group of [tex]5.27\times 10^{12}M_\odot[/tex], or [tex]\log M_{LG}/M_\odot = 12.72[/tex], with an interquartile range of [12.58, 12.83] and a 5% to 95% range of [12.26, 13.01]. Thus a 95% lower confidence limit on the true mass of the Local Group is [tex]1.81\times 10^{12}M_\odot[/tex]. A timing estimate of the Milky Way's mass based on the large recession velocity observed for the distant satellite Leo I works equally well, although with larger systematic uncertainties. It gives an estimated virial mass for the Milky Way of [tex]2.43 \times 10^{12}M_\odot[/tex] with a 95% lower confidence limit of [tex]0.80 \times 10^{12}M_\odot[/tex]."some comments:
Simon White is a top astrophysicist
it isn't easy to estimate the mass of Milky including her dark matter halo
the method that they used to estimate the masses is very beautiful and unlike anything i ever saw before
it involves using a computer simulation (the Millennium simulation) in which 8 billion dark matter chunks (each weighing a billion solar) cruise around under the influence of gravity, inside a large cubic box.

The estimate of the local group mass (mainly the mass of Andromeda+Milky) is 5 trillion solar.
Milky is a little bit under half of that.
 
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Related to Recent mass estimates for Milky and the Local Group

1. What is the significance of recent mass estimates for the Milky Way and the Local Group?

The recent mass estimates for the Milky Way and the Local Group are significant because they provide us with a better understanding of the structure and evolution of our own galaxy and its neighboring galaxies. They also help us to better understand the distribution and dynamics of dark matter within these systems.

2. How were these mass estimates calculated?

These mass estimates were calculated using a variety of methods, including kinematic measurements of stars and gas, gravitational lensing, and simulations. Each method has its own strengths and limitations, so combining multiple techniques allows for a more accurate estimation of the mass.

3. How do these new estimates compare to previous ones?

The new mass estimates for the Milky Way and the Local Group are generally higher than previous estimates. This is due to advancements in technology and techniques, as well as a better understanding of the complexities of galaxy formation and evolution.

4. What implications do these mass estimates have for our understanding of the universe?

The mass estimates for the Milky Way and the Local Group have significant implications for our understanding of the universe. They provide valuable insights into the distribution and composition of dark matter, the formation and evolution of galaxies, and the overall structure and dynamics of the universe.

5. How will these mass estimates be used in future research?

The mass estimates for the Milky Way and the Local Group will be used in future research to further our understanding of galaxy formation and evolution, dark matter, and the larger structures of the universe. They will also serve as important benchmarks for testing and refining current theories and models.

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