< iframe size="425 "height=" 355 "src =" https://www.youtube.com/embed/LyIEd5QVkyc?rel=0 "frameborder =" 0" allowfullscreen > Stephen takes a deep study the hack of the enormous credit report company Equifax, which might have revealed approximately 143 million people’s identifications.

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< iframe width =" 425" elevation =" 355" src =" https://www.youtube.com/embed/bvHIrTc08r0?rel=0 "frameborder =" 0" allowfullscreen > Krebs’ Blog Write-up:.
https://krebsonsecurity.com/2017/09/equifax-breach-response-turns-dumpster-fire/.

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” Take Control of Your Credit Today! ”
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< iframe width =" 425" elevation= "355" src= "https://www.youtube.com/embed/071XkCQyotM?rel=0" frameborder= "0" allowfullscreen > A very mad MotoMan & Kumo share the troubling news that vehicle loan exceeding 5 years has swollen from simply over 10% 7 years ago to more compared to a THIRD of all brand-new vehicle loan in the United States!!!! MotoMan soothes down for enough time to share additional understanding right into this unfavorable fad he gained from his local market and clarifies from a car individual’s viewpoint why this is trouble for your total assets …

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Latest 3 Credit Reports News

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Supernova Remnant is a Textbook Case (NASA, Chandra, 1/30/07)
3 credit reports
Image by NASA’s Marshall Space Flight Center
Editor’s Note: This image from 2007 shows Chandra X-ray & VLA Radio Images of G11.2-0.3.

G11.2-0.3 is a circularly symmetric supernova remnant that contains a dense, rotating dead star at its center, representing a textbook case of what the remnant of an exploding star should look like after a couple thousand years. When a massive star collapses, the outer layers of the star are blown away in an extremely energetic explosion. Depending on the mass of the original star, a dense object such as a neutron star or a black hole, can form and be left behind at the explosion’s center. Such a neutron star, known as a "pulsar" when it rapidly rotates, can be kicked by the thermonuclear shock wave created when the star exploded, causing it to race through space at millions of miles per hour.

By combining X-ray and radio observations, astronomers have evidence that G11.2-0.3 is likely the result of the explosive death of such a massive star, perhaps witnessed in 386 A.D. Radio observations measure the remnant’s expansion rate, which, in turn, can be used to calculate how long ago the star exploded. The radio data is consistent with association of the supernova remnant with the "guest star" reported by Chinese astronomers nearly 2,000 years ago. Chandra’s ability to pinpoint the pulsar at nearly the very center of G11.2-0.3 also supports the idea that this debris field could have been created around the time of the Chinese observations. Surprisingly, the age of the pulsar determined from the X-ray and radio data differs from the standard pulsar age estimate, usually determined from how fast it is spinning. In this case, the so-called spin parameters suggest the G11.2-0.3 is 10 times older than the remnant age. This argues strongly that young pulsar spin ages can be very misleading and should be considered with caution.

Read entire caption/view more images: www.chandra.harvard.edu/photo/2007/g11/

Image credit: X-ray: NASA/CXC/Eureka Scientific/M.Roberts et al.; Radio: NRAO/AUI/NSF

Caption credit: Harvard-Smithsonian Center for Astrophysics

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Choices for renting a flat in Brooklyn for those who have bad credit.

What Credit Bureaus DON’T Want You to Know!

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http://creditrepairpublishing.com/credit-repair-articles/56-credit-bureaus/151-what-the-credit-bureaus-dont-want-you-to-know-about-the-metro-2-format-and-credit-reporting
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