Abstract
We present the results of two studies of the inner Galaxy : on the one hand, a maximum likelihood fitting method using the Besançon model of Galaxy to constrain the density laws of the outer bulge and the holed disc; on the other hand, the comparison of Besançon simulations with infrared data on fields near longitude 20–27 degrees to verify the existence of a long and thin in-plane bar. These two parallel studies seem to show the co-existence of a structure (the bar) in addition with a very oblate outer bulge.
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Picaud, S., Chereul, E., Robin, A.C. et al. Outer bulge and in-plane bar of the milky way. Astrophysics and Space Science 284, 523–526 (2003). https://doi.org/10.1023/A:1024020714722
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DOI: https://doi.org/10.1023/A:1024020714722