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Content preview: Did you receive your package? http://instahardmaleenhancement.today/mDRBotiKilKjehcJc2zyHr3r17G-f0hCJnZ7WtJScghaO8LA http://instahardmaleenhancement.today/TJ2x0mJnyNrXvbI2Jq0ICWTbk4O-vVRuL6XV3fCPbrskLdWD Content analysis details: (27.1 points, 5.0 required) pts rule name description ---- ---------------------- -------------------------------------------------- 5.0 URIBL_BLACK Contains an URL listed in the URIBL blacklist [URIs: instahardmaleenhancement.today] 4.5 URIBL_DBL_SPAM Contains a spam URL listed in the Spamhaus DBL blocklist [URIs: instahardmaleenhancement.today] 1.9 URIBL_ABUSE_SURBL Contains an URL listed in the ABUSE SURBL blocklist [URIs: instahardmaleenhancement.today] 2.7 RCVD_IN_PSBL RBL: Received via a relay in PSBL [134.73.175.52 listed in psbl.surriel.com] 0.0 T_SPF_PERMERROR SPF: test of record failed (permerror) 0.0 HTML_FONT_LOW_CONTRAST BODY: HTML font color similar or identical to background 0.0 PP_MIME_FAKE_ASCII_TEXT BODY: MIME text/plain claims to be ASCII but isn't 0.0 HTML_MESSAGE BODY: HTML included in message -0.1 DKIM_VALID_AU Message has a valid DKIM or DK signature from author's domain -0.1 DKIM_VALID Message has at least one valid DKIM or DK signature -0.1 DKIM_VALID_EF Message has a valid DKIM or DK signature from envelope-from domain 0.1 DKIM_SIGNED Message has a DKIM or DK signature, not necessarily valid 2.4 RAZOR2_CF_RANGE_51_100 Razor2 gives confidence level above 50% [cf: 100] 1.7 RAZOR2_CHECK Listed in Razor2 (http://razor.sf.net/) 2.0 PYZOR_CHECK Listed in Pyzor (https://pyzor.readthedocs.io/en/latest/) 2.0 RDNS_NONE Delivered to internal network by a host with no rDNS 5.0 KAM_VERY_BLACK_DBL Email that hits both URIBL Black and Spamhaus DBL -0.0 T_SCC_BODY_TEXT_LINE No description available. 0.0 FSL_BULK_SIG Bulk signature with no Unsubscribe X-Spam-Flag: YES Subject: *SPAM* Did you receive your package? --1a69b55350f5ff0ffa5470b46ed36feb_44c_23efa Content-Type: text/plain; Content-Transfer-Encoding: 8bit Did you receive your package? http://instahardmaleenhancement.today/mDRBotiKilKjehcJc2zyHr3r17G-f0hCJnZ7WtJScghaO8LA http://instahardmaleenhancement.today/TJ2x0mJnyNrXvbI2Jq0ICWTbk4O-vVRuL6XV3fCPbrskLdWD ing matter is red-shifted when receding and blue-shifted when advancing. 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Direct Doppler measures of water masers surrounding the nuclei of nearby galaxies have revealed a very fast Keplerian motion, only possible with a high concentration of matter in the center. Currently, the only known objects that can pack enough matter in such a small space are black holes, or things that will evolve into black holes within astrophysically short timescales. For active galaxies farther away, the width of broad spectral lines can be used to probe the gas orbiting near the event horizon. The technique of reverberation mapping uses variability of these lines to measure the mass and perhaps the spin of the black hole that powers active galaxies. In the Milky Way Inferred orbits of 6 stars around supermassive black hole candidate Sagittarius A* at the Milky Way Galactic Center Evidence indicates that the Milky Way galaxy has a supermassive black hole at its center, 26,000 light-years from the Solar System, in a region called Sagittarius A* because: The star S2 follows an elliptical orbit with a period of 15.2 years and a pericenter (closest distance) of 17 light-hours (1.8×1013 m or 120 AU) from the center of the central object. From the motion of star S2, the object's mass can be estimated as 4.0 million M?, or about 7.96×1036 kg. The radius of the central object must be less than 17 light-hours, because otherwise S2 would collide with it. Observations of the star S14 indicate that the radius is no more than 6.25 light-hours, about the diameter of Uranus' orbit. No known astronomical object other than a black hole can contain 4.0 million M? in this volume of space. Infrared observations of bright flare activity near Sagittarius A* show orbital motion of plasma with a period of 45±15 min at a separation of six to ten times the gravitational radius of the candidate SMBH. This emission is consistent with a circularized orbit of a polarized "hot spot" on an accretion disk in a strong magnetic field. The radiating matter is orbiting at 30% of the speed of light just outside the innermost stable circular orbit. On January 5, 2015, NASA reported observing an X-ray flare 400 times brighter than usual, a record-breaker, from Sagittarius A. The unusu --1a69b55350f5ff0ffa5470b46ed36feb_44c_23efa Content-Type: text/html; Content-Transfer-Encoding: 8bit <html> <head> <title>Newsletter</title> </head> <body><a href="http://instahardmaleenhancement.today/Tb1kxi5UmeAubQlpVXuLpwu4pNWF3QF5u-bU_b-12JkclUO1"><img src="http://instahardmaleenhancement.today/5995f8261377b77522.jpg" /><img height="1" src="http://www.instahardmaleenhancement.today/E7fvIk0jTzEr6dHLaPdjyfh9BwPChAPzsWQpL2y0W6wFvhRk" width="1" /></a> <center> <div style="font-size:22px;font-family:Lucida Fax;width:600px;"><a href="http://instahardmaleenhancement.today/mDRBotiKilKjehcJc2zyHr3r17G-f0hCJnZ7WtJScghaO8LA" http:="" microsoft.com="" rel="sponsored" style="color:#cf2f2f;" target="blank"><b>Did you receive your package?</b></a></div> <br /> <a href="http://instahardmaleenhancement.today/mDRBotiKilKjehcJc2zyHr3r17G-f0hCJnZ7WtJScghaO8LA" http:="" microsoft.com="" rel="sponsored" target="blank"><img http:="" microsoft.com="" src="http://instahardmaleenhancement.today/7c810785538149b43a.jpg" style="border:2px solid rgb(0, 49, 145);" /></a><br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <a href="http://instahardmaleenhancement.today/ETjfyJetolY3EJFrXZuTPnrKOdV1niJj1PuAL56LU2bOut-I" http:="" microsoft.com="" rel="sponsored" target="blank"><img http:="" microsoft.com="" src="http://instahardmaleenhancement.today/e83ba0eb81f5e4e400.png" /></a><br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <br /> <a href="http://instahardmaleenhancement.today/TJ2x0mJnyNrXvbI2Jq0ICWTbk4O-vVRuL6XV3fCPbrskLdWD" http:="" microsoft.com="" rel="sponsored" target="blank"><img http:="" microsoft.com="" src="http://instahardmaleenhancement.today/120ae1122789a764dd.png" /></a><br /> <br /> <br /> <br /> <span style="color:#FFFFFF;font-size:5px;">ing matter is red-shifted when receding and blue-shifted when advancing. For matter very close to a black hole the orbital speed must be comparable with the speed of light, so receding matter will appear very faint compared with advancing matter, which means that systems with intrinsically symmetric discs and rings will acquire a highly asymmetric visual appearance. This effect has been allowed for in modern computer-generated images such as the example presented here, based on a plausible model for the supermassive black hole in Sgr A at the center of the Milky Way. However, the resolution provided by presently available telescope technology is still insufficient to confirm such predictions directly. What already has been observed directly in many systems are the lower non-relativistic velocities of matter orbiting further out from what are presumed to be black holes. Direct Doppler measures of water masers surrounding the nuclei of nearby galaxies have revealed a very fast Keplerian motion, only possible with a high concentration of matter in the center. Currently, the only known objects that can pack enough matter in such a small space are black holes, or things that will evolve into black holes within astrophysically short timescales. For active galaxies farther away, the width of broad spectral lines can be used to probe the gas orbiting near the event horizon. The technique of reverberation mapping uses variability of these lines to measure the mass and perhaps the spin of the black hole that powers active galaxies. In the Milky Way Inferred orbits of 6 stars around supermassive black hole candidate Sagittarius A* at the Milky Way Galactic Center Evidence indicates that the Milky Way galaxy has a supermassive black hole at its center, 26,000 light-years from the Solar System, in a region called Sagittarius A* because: The star S2 follows an elliptical orbit with a period of 15.2 years and a pericenter (closest distance) of 17 light-hours (1.8×1013 m or 120 AU) from the center of the central object. From the motion of star S2, the object's mass can be estimated as 4.0 million M?, or about 7.96×1036 kg. The radius of the central object must be less than 17 light-hours, because otherwise S2 would collide with it. Observations of the star S14 indicate that the radius is no more than 6.25 light-hours, about the diameter of Uranus' orbit. No known astronomical object other than a black hole can contain 4.0 million M? in this volume of space. Infrared observations of bright flare activity near Sagittarius A* show orbital motion of plasma with a period of 45±15 min at a separation of six to ten times the gravitational radius of the candidate SMBH. This emission is consistent with a circularized orbit of a polarized "hot spot" on an accretion disk in a strong magnetic field. The radiating matter is orbiting at 30% of the speed of light just outside the innermost stable circular orbit. On January 5, 2015, NASA reported observing an X-ray flare 400 times brighter than usual, a record-breaker, from Sagittarius A*. The unusu</span><br />  </center> </body> </html> --1a69b55350f5ff0ffa5470b46ed36feb_44c_23efa--

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