- #1
betzalel
- 64
- 5
There is a confusing article in the August, 2012 Scientific America concerning the recent discovery of a massive gamma radiation emission from the Milky Way galaxy, from the very recent past. As our solar system is one of the many members of the Milky Way this is an interesting subject.
If viewed from a distance galaxy, say M31, this massive gamma radiation emission would appear to be a Quasar, a QSO, a quasi-stellar object. As there are no QSOs in the local universe this presents an interesting puzzle. Why are there no QSOs in the local universe and how the heck can there be a QSO in the Milky Way?
To have an intelligent conversation concerning the Milky Way's hypothesized QSO it is necessary to review the observational evidence concerning QSOs. i.e. One can compare the toy model for QSOs to the observations and see if the observations match what is observed.
http://arxiv.org/pdf/1205.5852v1.pdf
If viewed from a distance galaxy, say M31, this massive gamma radiation emission would appear to be a Quasar, a QSO, a quasi-stellar object. As there are no QSOs in the local universe this presents an interesting puzzle. Why are there no QSOs in the local universe and how the heck can there be a QSO in the Milky Way?
To have an intelligent conversation concerning the Milky Way's hypothesized QSO it is necessary to review the observational evidence concerning QSOs. i.e. One can compare the toy model for QSOs to the observations and see if the observations match what is observed.
http://arxiv.org/pdf/1205.5852v1.pdf
Evidence for Gamma Ray Jets in the Milky Way
Although accretion onto supermassive black holes in other galaxies is seen to produce powerful jets in X-ray and radio, no convincing detection has ever been made of a kpc-scale jet in the Milky Way. The recently discovered pair of 10 kpc tall gamma-ray bubbles in our Galaxy may be signs of earlier jet activity from the central black hole. In this paper, we identify a gamma-ray cocoon feature in the southern bubble, a jet-like feature along the cocoon’s axis of symmetry, and another directly opposite the Galactic center in the north. Both the cocoon and jet-like feature have a hard spectrum with spectral index _ −2 from 1 to 100 GeV, with a cocoon total luminosity of (5.5 ± 0.45) × 10^35 and luminosity of the jet-like feature of (1.8 ± 0.35) × 10^35 erg/s at 1 − 100 GeV. If confirmed, these jets are the first resolved gamma-ray jets ever seen.
The mechanism by which jets turn on and off is one of the major puzzles in high energy astrophysics, and may be connected to star formation (Antonuccio-Delogu & Silk 2008). The relativistic jets inject significant amounts of energy into the medium within which they propagate, creating an extended, under-dense and hot cocoon. After decades of study, we still lack a complete understanding of the main mechanism launching, accelerating, and collimating jets, with limited knowledge of the energy content, the composition, and the particle acceleration mechanisms of the jets (Blandford & Znajek 1977; Blandford & Payne 1982)...
...The SMBH at the center of the Milky Way (MW) is surrounded by clusters of young stars and giant molecular clouds (Morris & Serabyn 1996). Although there are indications of past activity (Sunyaev et al. 1993), the SMBH is currently in a quiescent state. Despite the abundant observational evidence of large-scale jets in other galaxies, it was not expected that the Milky Way’s SMBH would produce such a relativistic collimated structure, given its current quiescence. However, the MW must have undergone phases of nuclear activity in the past in order for the SMBH to grow, and it is plausible that signs of past activity are still visible.