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Trader 1 from Vienna – YouTube

Be obsessed or be average. – Grant Cardone #10X

//Recommended Books by Grant Cardone: Author of The 10X Rule + Be Obsessed Or Be Average

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Trade Historical Data and Save Your Time

This Forex Simulator lets you move back in time and replay the market starting from any selected day. It shows you charts, indicators and economic news as if it was happening live. You are able to place your orders, modify them or close them, just like you were trading live.

Trading historical data saves a lot of time compared to demo trading and other forms of paper trading. It also allows to adjust the speed of simulation, so you can skip less important periods of time and focus on the most important ones.

Understand Price Action & Market Structure.

Works on Multiple Timeframes

You can open several charts at once and follow price action on several timeframes. You can also create custom timeframe charts, like 10-minute chart or 2-day chart. All charts are synchronized and updated tick-by-tick.

Forex Simulator - Multiple timeframes

How it works

Forex Simulator works as Expert Advisor for Metatrader 4. It combines great charting capabilities of MT4 with quality tick-by-tick data and economic calendar to create a powerful trading simulator. It uses offline charts, which let you use indicators, templates and drawing tools available in Metatrader.

Multiple timeframes

However, it is not limited to using historical data offered by Metatrader, which is usually low-quality data. It also lets you download and use high-quality tick data from Dukascopy and TrueFX.

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FOREX & CFDs trading are complex instruments and come with a high risk of losing money rapidly due to leverage. 78.8 % of retail investor accounts lose money when trading FOREX & CFDs



Star clusters are commonly featured in cosmic photoshoots, and are also well-loved by the keen eye of the NASA/ESA Hubble Space Telescope. These large gatherings of celestial gems are striking sights — and the subject of this Picture of the Week, Messier 2, is certainly no exception. Messier 2 is located in the constellation of Aquarius (The Water-Bearer), about 55 000 light-years away. It is a globular cluster, a spherical group of stars all tightly bound together by gravity. With a diameter of roughly 175 light-years, a population of 150 000 stars, and an age of 13 billion years, Messier 2 is one of the largest clusters of its kind and one of the oldest associated with the Milky Way. Most of the cluster’s mass is concentrated at its centre, with shimmering streams of stars extending outwards into space. It is bright enough that it can even be seen with the naked eye when observing conditions are extremely good.
Planetary nebulae represent the final, brief stage in the life of a medium-sized star like our Sun. While consuming the last of the fuel in its core, the dying star expels a large portion of its outer envelope. This material is then illuminated by the ultraviolet radiation from the stellar remnant, producing glowing clouds of gas that can show complex structure.
A spectacular example of this beautiful complexity is seen in the bluish lobes of NGC 5189. Most of the nebula is knotty and filamentary in its structure. As a result of the mass-loss process, the planetary nebula has been created with two nested structures, tilted with respect to each other, that expand away from the center in different directions. The bright golden ring that twists and tilts through the nebula is made up of a large collection of radial filaments and cometary knots. These are usually formed by the combined action of photo-ionizing radiation and stellar winds.
The nebula is located 1,800 light-years away in the southern constellation Musca. Hubble’s image is the most detailed yet made of this object. Its double bipolar or quadrupolar structure could be explained by the presence of a second star orbiting the central star and influencing the pattern of mass ejection during its nebula-producing death throes. The remnant of the central star, having lost much of its mass, now lives its final days as a white dwarf. However, there is no visual candidate for the possible companion.
The name „planetary nebulae“ originated with astronomers who studied them through early telescopes with little magnification and optics that were far from sharp. The brightly colored nebulae are often roughly spherical, and many appear green or blue like Uranus and Neptune at lower resolution, so their appearance evoked that of the giant planets in the outer solar system. Many do look somewhat planet-like, but not NGC 5189. This nebula forms a dramatic reverse S-shape.
Planetary nebulae tell us about the possible fate of the Sun, which may form such a nebula when it runs out of fuel in a little over 5 billion years. In 2012, Sze-Ning Chong of Japan’s Kagoshima University and collaborators used Hubble data to study the three-dimensional shapes of 20 complex planetary nebulae, including NGC 5189, and determined that a multipolar nebula with at least three pairs of lobes could explain many of the features in NGC 5189.
In 2014, Graziela R. Keller of the University of Sao Paulo in Brazil also used Hubble data to study the characteristics of the light and wind emitted from planetary nebulae, including NGC 5189. She studied the chemical composition of NGC 5189’s central star and discovered significantly more nitrogen than previously estimated. The larger amount of nitrogen suggests that the star went through an outburst phase that contributed to the formation of the complex structure seen in the image. The different lobes may each come from a separate outburst in the distant past.
Constellation: Musca
Distance: 1,800 light-years
The Great Observatories‘ Multiwavelength View of the Crab Nebula
This new multiwavelength image of the Crab Nebula combines X-ray light from the Chandra X-ray Observatory (in blue) with visible light from the Hubble Space Telescope (in yellow) and infrared light seen by the Spitzer Space Telescope (in red). This particular combination of light from across the electromagnetic spectrum highlights the nested structure of the pulsar wind nebula.
The X-rays reveal the beating heart of the Crab, the neutron-star remnant from the supernova explosion seen almost a thousand years ago. This neutron star is the super-dense collapsed core of an exploded star and is now a pulsar that rotates at a blistering rate of 30 times per second. A disk of X-ray-emitting material, spewing jets of high-energy particles perpendicular to the disk, surrounds the pulsar. The infrared light in this image shows synchrotron radiation, formed from streams of charged particles spiraling around the pulsar’s strong magnetic fields.
The visible light is emission from oxygen that has been heated by higher-energy (ultraviolet and X-ray) synchrotron radiation. The delicate tendrils seen in visible light form what astronomers call a „cage“ around the rich tapestry of synchrotron radiation, which in turn encompasses the energetic fury of the X-ray disk and jets. These multiwavelength interconnected structures illustrate that the pulsar is the main energy source for the emission seen by all three telescopes.
The Crab Nebula resides 6,500 light-years from Earth in the constellation Taurus.


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