From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #11342 Reply-To: ammf@fruvous.com Sender: owner-ammf-digest@smoe.org Errors-To: owner-ammf-digest@smoe.org Precedence: bulk alt.music.moxy-fruvous digest Saturday, May 13 2023 Volume 14 : Number 11342 Today's Subjects: ----------------- Herpes Virus Hiding Place Revealed! (Nobody Believed This!) ["Cold sore v] ---------------------------------------------------------------------- Date: Sat, 13 May 2023 11:25:50 +0200 From: "Cold sore virus" Subject: Herpes Virus Hiding Place Revealed! (Nobody Believed This!) Herpes Virus Hiding Place Revealed! (Nobody Believed This!) http://malenhancement.live/4SaRVP_EUaq9zGlSdPB0gbusNsx_-5OP3IVKsJVc03zM7gHzzQ http://malenhancement.live/oS86yMiDUUjD5A9SudyNdyjWuQGxPootPZArxji0kxM4bsKQyQ iguous dynamical evidence for supermassive black holes exists only for a handful of galaxies; these include the Milky Way, the Local Group galaxies M31 and M32, and a few galaxies beyond the Local Group, such as NGC 4395. In these galaxies, the root mean square (or rms) velocities of the stars or gas rises proportionally to 1/r near the center, indicating a central point mass. In all other galaxies observed to date, the rms velocities are flat, or even falling, toward the center, making it impossible to state with certainty that a supermassive black hole is present. Nevertheless, it is commonly accepted that the center of nearly every galaxy contains a supermassive black hole. The reason for this assumption is the Mbsigma relation, a tight (low scatter) relation between the mass of the hole in the 10 or so galaxies with secure detections, and the velocity dispersion of the stars in the bulges of those galaxies. This correlation, although based on just a handful of galaxies, suggests to many astronomers a strong connection between the formation of the black hole and the galaxy itself. On March 28, 2011, a supermassive black hole was seen tearing a mid-size star apart. That is the only likely explanation of the observations that day of sudden X-ray radiation and the follow-up broad-band observations. The source was previously an inactive galactic nucleus, and from study of the outburst the galactic nucleus is estimated to be a SMBH with mass of the order of a million M?. This rare event is assumed to be a relativistic outflow (material being emitted in a jet at a significant fraction of the speed of light) from a star tidally disrupted by the SMBH. A significant fraction of a solar mass of material is expected to have accreted onto the SMBH. Subsequent long-term observation will allow this assumption to be confirmed if the emission from the jet decays at the expected rate for mass accretion onto a SMBH. Individual studies Hubble Space Telescope photograph of the 4,400 light-year-long relativistic jet of Messier 87, which is matter being ejected by the 6.5C109 M? supermassive black hole at the center of the galaxy The nearby Andromeda Galaxy, 2.5 million light-years away, contains a 1.4+0.65 ?0.45C108 (140 million) M? central black hole, significantly larger than the Milky Way's. The largest supermassive black hole in the Milky Way's vicinity appears to be that of Messier 87 (i.e., M87*), at a mass of (6.5B10.7)C109 (c. 6.5 billion) M? at a distance of 48.92 million light-years. The supergiant elliptical galaxy NGC 4889, at a distance of 336 million light-years away in the Coma Berenices constellation, contains a black hole measured to be 2.1+3.5 ?1.3C1010 (21 billion) M?. Masses of bl ------------------------------ End of alt.music.moxy-fruvous digest V14 #11342 ***********************************************