Milky Way tagged posts

Computer Simulations Shed Light on the Milky Way’s Missing Red Giants

A sequence of snapshots from a simulation showing a red giant star tunneling through a high density gas clump. The star is moving downward in the illustration, as indicated by the bow-shaped "onion skin" surfaces of constant density. Soon after the star plunges into the clump, it develops a high temperature "blister" at the point of impact and a full turbulent wake behind it. Credit: Georgia Tech

A sequence of snapshots from a simulation showing a red giant star tunneling through a high density gas clump. The star is moving downward in the illustration, as indicated by the bow-shaped “onion skin” surfaces of constant density. Soon after the star plunges into the clump, it develops a high temperature “blister” at the point of impact and a full turbulent wake behind it. Credit: Georgia Tech

Why is the center of the Milky Way filled with young stars but has very few old ones. According to the theory, the remnants of older, red giant stars are still there – they just aren’t bright enough to be detected with telescopes...

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ATLASGAL Survey of Milky Way completed

This part image of the Milky Way has been released to mark the completion of the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). The APEX telescope in Chile has mapped the full area of the Galactic Plane visible from the southern hemisphere for the first time at submillimeter wavelengths -- between infrared light and radio waves -- and in finer detail than recent space-based surveys. The APEX data, at a wavelength of 0.87 millimeters, shows up in red and the background blue image was imaged at shorter infrared wavelengths by the NASA Spitzer Space Telescope as part of the GLIMPSE survey. The fainter extended red structures come from complementary observations made by ESA's Planck satellite. The full-resolution image is available on the ESO web page: https://www.eso.org/public/images/eso1606a/ Credit: ESO/APEX/ATLASGAL consortium/NASA/GLIMPSE consortium/ESA/Planck

This part image of the Milky Way has been released to mark the completion of the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). The APEX telescope in Chile has mapped the full area of the Galactic Plane visible from the southern hemisphere for the first time at submillimeter wavelengths — between infrared light and radio waves — and in finer detail than recent space-based surveys. The APEX data, at a wavelength of 0.87 millimeters, shows up in red and the background blue image was imaged at shorter infrared wavelengths by the NASA Spitzer Space Telescope as part of the GLIMPSE survey. The fainter extended red structures come from complementary observations made by ESA’s Planck satellite. The full-resolution image is available on the ESO web page: https://www.eso...

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Monstrous Cloud Boomerangs back to our Galaxy

This composite image shows the size and location of the Smith Cloud on the sky. The cloud appears in false-color, radio wavelengths as observed by the Robert C. Byrd Green Bank Telescope in West Virginia. The visible-light image of the background star field shows the cloud's location in the direction of the summer constellation Aquila. The cloud is 15 degrees across in angular size -- the width of an outstretched hand at arm's length. The apparent size of the full moon is added for comparison. Credit: B. Saxton and F. Lockman (NRAO/AUI/NSF), and A. Mellinger

This composite image shows the size and location of the Smith Cloud on the sky. The cloud appears in false-color, radio wavelengths as observed by the Robert C. Byrd Green Bank Telescope in West Virginia. The visible-light image of the background star field shows the cloud’s location in the direction of the summer constellation Aquila. The cloud is 15 degrees across in angular size — the width of an outstretched hand at arm’s length. The apparent size of the full moon is added for comparison. Credit: B. Saxton and F. Lockman (NRAO/AUI/NSF), and A. Mellinger

New Hubble telescope observations suggest a high-velocity H gas cloud was launched from the outer regions of our own galaxy around 70 million years ago...

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“Cosmic Archeological Dig” of Milky Way’s heart, uncovers Blueprints of Early Construction Phase

White dwarf stars in the early Milky Way. Credit: NASA, ESA, A. Calamida and K. Sahu (STScI), and the SWEEPS Science Team; Credit for Ground-based Image: A. Fujii

White dwarf stars in the early Milky Way. Credit: NASA, ESA, A. Calamida and K. Sahu (STScI), and the SWEEPS Science Team; Credit for Ground-based Image: A. Fujii

Peering deep into the Milky Way’s crowded central hub of stars, Hubble researchers have uncovered for the 1st time a population of ancient white dwarfs, smoldering remnants of once-vibrant stars that inhabited the core. This can yield clues to how our galaxy was built, long before Earth/sun formed.

The white dwarfs contain information about the stars that existed about 12 billion years ago that burned out to form the white dwarfs. As these dying embers of once-radiant stars cool, they serve as multi-billion-year-old time pieces that tell astronomers about the Milky Way’s groundbreaking years.

An analysis of the Hubble data suppor...

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