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The pervasiveness of O 6 absorption lines, coupled with complementary observations of a diffuse background in soft X-rays and EUV radiation, shows that there is an extensive network of low density gas (n approx. Observations of these features which have been very influential in revising the perception of the medium's various physical states, are discussed. In the ultraviolet spectra of hot stars, absorption lines can be seen from highly ionized species in the interstellar medium. Observations of Absorption Lines from Highly Ionized Atoms The amount of observable emission and polarization expected to be produced by the BAL clouds from resonance line scattering and collisional excitation is considered in This suggests that possibly all, but not less than 15 percent, of the QSOs have BAL clouds associated with them. By considering the observed percentage of QSOs with BALs and resonance line scattering models, it is found that the absorption covering factor in BAL QSOs is between 3 and 20 percent. Also, photoionization models, which utilize solar abundances and take the ionizing continuum to be a simple power law, are incapable of explaining the level of ionization in the BAL clouds. Therefore, if the BAL clouds give rise to observable emission, the generally adopted (optically thick, single component) model for the emission line region must be incorrect. The BAL clouds are incapable of accounting for all of the observed broad emission lines, particularly C III} (lamda)1909 and Mg II (lamda)2798. The distribution of multiplicities for isolated absorption troughs suggests that the large -scale spatial distribution of BAL clouds is non-random, possibly described by a disk geometry.
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For example, N V emission is generally stronger in BAL QSOs and the emission near C III} (lamda)1909 is generally broader in BAL QSOs. The emission line properties of BAL QSOs appear to be different from those of non-BAL QSOs.
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The minimum total absorption column densities are 10('20) to 10('22) cm('-2). Outflow velocities up to 40,000 km s(' -1) are observed. The BALs exhibit a variety of velocity structures, from seemingly smooth, continuous absorption to complexes of individual absorption lines. Broad absorption lines (BALs) are probably present in 3 to 10 percent of the spectra of moderate to high redshift QSOs.
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The following major conclusions are reached. Spectroscopic observations of fourteen broad absorption line (BAL) QSOs are presented and analyzed. the music.Broad Absorption Lines in Qsos: Observations and Implications for Models. A love letter between the Japanese fans who were living under the umbrella of recent tragedy, and the band who simply, while after being warned not to go there, went to heal with the only medicine they could. This film directed by Casey Patrick Tebo, documents both the performances and the band’s relationship with Japan. Landing in Tokyo just 6 months after Fukushima, Aerosmith began the Japanese leg of their world tour in devastating circumstances. More than anything else it demonstrates the Japanese fans love affair with Aerosmith and their music.
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This film follows the band on that tour combining full length live tracks with behind the scenes footage which is at times touching and emotional and at others humorous and insightful. The Japanese fans came out in their droves and Aerosmith responded with some of the finest gigs of their distinguished career. In the fall of 2011, despite advice to the contrary, Aerosmith brought their Back On The Road tour to Japan, a country with which they'd always had a special relationship. In March 2011 Japan was beset by a huge earthquake, a monstrous tsunami and the subsequent meltdown of the Fukushima nuclear plant. A new video clip of their hit 'Love In An Elevator' can be viewed below: “I sincerely hope Aerosmith will get another opportunity to come back to Shanghai and Taiwan to play for our many fans there.”Īerosmith's Rock For The Rising Sun concert film follows the Bad Boys from Boston across Japan in the months after the devastating nuclear meltdown, and was released on DVD and Blu-Ray this week via Eagle Rock Entertainment. “I'm disappointed we weren't able to play for our fans in China however, the circumstances were beyond our control,” says Joey Kramer. “We were really looking forward to visiting Shanghai and Taipei and playing for our fans there and are very disappointed that these two shows have been cancelled.” “It's always been a dream of ours to play in Shanghai and Taipei, and meet our fans there," Tom Hamilton says. “We've looked forward to this for a lifetime.” “We're disappointed as we wanted to play for our fans,” said Joe Perry.