Tag Archive for 'Galaxy'

This composite image, which combines infrared (blue), radio (red) and microwave (green) observations from the GISMO instrument, reveals emission from cold dust, areas of vigorous star formation, and filaments formed at the edges of a bubble blown by some powerful event at the Milky Way Galaxy’s center. Image credit: NASA’s Goddard Space Flight Center.

GISMO Sees Huge Molecular Clouds and Filaments in Milky Way’s Central Region

Dec 18, 2019 by News Staff

The NASA-designed Goddard-IRAM Superconducting 2-Millimeter Observer (GISMO), a bolometer camera installed on the 30-m IRAM radio telescope, has produced...

This image, taken by Hubble’s Advanced Camera for Surveys (ACS) on July 18, 2019, shows NGC 1175. Image credit: NASA / ESA / Hubble Team.

Hubble Space Telescope Looks at Stunning Peanut Galaxy

Dec 17, 2019 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured an amazing photo of a galaxy called NGC 1175. This image, taken by Hubble’s Advanced...

An artist’s impression of a carbon halo around a young star-forming galaxy. Image credit: National Astronomical Observatory of Japan.

ALMA Spots Carbon Halos around Early Star-Forming Galaxies

Dec 17, 2019 by Enrico de Lazaro

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have spotted huge clouds of carbon gas around several young starburst galaxies...

Taken with the HAWK-I instrument on ESO’s Very Large Telescope, this stunning image shows the Milky Way’s central region with an angular resolution of 0.2 arcseconds. The image combines observations in three different wavelength bands. Image credit: ESO / Nogueras-Lara et al.

VLT Observes Milky Way’s Central Region

Dec 16, 2019 by News Staff

Astronomers using ESO’s Very Large Telescope (VLT) have captured a stunning new image of the Milky Way’s densest region of stars, gas and dust, which...

An artistic illustration of a binary black hole. Image credit: NASA / ESA / G. Bacon, STScI.

Milky Way’s Central Black Hole May Have a Supermassive Companion

Dec 16, 2019 by The Conversation

Do supermassive black holes have friends? The nature of galaxy formation suggests that the answer is yes, and in fact, pairs of supermassive black holes...

This Hubble image shows the central region of IC 2051, a spiral galaxy located 90 million light-years away in the constellation Mensa. The image is made up of observations from Hubble’s Wide Field Camera 3 (WFC3) in the optical and infrared parts of the spectrum. Three filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / P. Erwin et al.

Hubble Snaps Close-Up of Spiral Galaxy IC 2051

Dec 16, 2019 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope has captured an outstanding image of the central part of the compact spiral galaxy IC 2051. This Hubble image shows...

X-ray image of the gravitational lens system SDSS J1004+4112 taken by NASA’s Chandra X-ray Observatory; the central red extended emission is from the hot gas in the foreground lens galaxy cluster and the four blue point sources are the lensed images of the background quasar. Image credit: University of Oklahoma.

Free-Floating Planet-Mass Objects are Common in Galaxies

Dec 13, 2019 by Enrico de Lazaro

Using a technique called quasar microlensing, a team of astronomers at the University of Oklahoma has detected populations of free-floating planet-mass...

This image, taken by the Gemini Multi-Object Spectrograph on the Frederick C. Gillett Gemini North telescope, shows the interacting galaxy pair NGC 5394-NGC 5395. Image credit: NSF’s National Optical-Infrared Astronomy Research Laboratory / Gemini Observatory / AURA.

Gemini North Telescope Captures Stunning Galaxy Collision

Dec 13, 2019 by Enrico de Lazaro

Astronomers working at the NSF-supported Gemini Observatory have captured a new photo of interacting spiral galaxies NGC 5394 and NGC 5395, collectively...

Milky Way’s center produces more high-energy gamma rays than can be explained by known sources. This image shows the Milky Way in visible light and a gamma-ray map from NASA’s Fermi Gamma-ray Space Telescope. Image credit: NASA’s Goddard Space Flight Center / A. Mellinger, Central Michigan University / T. Linden, University of Chicago.

Annihilating Dark Matter May Lurk in Milky Way’s Center

Dec 12, 2019 by News Staff

Gamma rays — the most energetic waves in the electromagnetic spectrum — are typically produced by the hottest, most extreme objects in the...

Merging Pair of Dusty Star-Forming Galaxies Spotted 13 Billion Light-Years Away

Dec 12, 2019 by News Staff

Using the Atacama Large Millimeter/submillimeter Array (ALMA), an international team of astronomers has spotted an unlensed, dusty star-forming galaxy...

Magnetic fields in the spiral galaxy Messier 77, also known as M77 and NGC 1086, are shown as streamlines over a visible light and X-ray composite image of the galaxy from the NASA/ESA Hubble Space Telescope, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR), and the Sloan Digital Sky Survey. The magnetic fields align along the entire length of the massive spiral arms of Messier 77, implying that the gravitational forces that created the galaxy’s shape are also compressing the its magnetic field. This supports the leading theory of how the spiral arms are forced into their iconic shape known as ‘density wave theory.’ SOFIA studied the galaxy using far-infrared light (89 microns) to reveal facets of its magnetic fields that previous observations using visible and radio telescopes could not detect. Image credit: NASA / SOFIA / JPL-Caltech / Roma Tre University.

Magnetic Fields Play Important Role in Shaping Spiral Galaxies

Dec 11, 2019 by News Staff

New infrared observations from NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) of Messier 77, a spiral galaxy located 47 million light-years...

NGC 3175 can be seen slicing across the frame in this Hubble image, with its mix of bright patches of glowing gas, dark lanes of dust, bright core, and whirling, pinwheeling arms coming together to paint a beautiful celestial scene. This image is made up of observations from Hubble’s Wide Field Camera 3 (WFC3) in the infrared and optical parts of the spectrum. Two filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / D. Rosario et al.

Hubble Captures Detailed Image of Edge-On Spiral Galaxy NGC 3175

Dec 9, 2019 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope has delivered an incredible snapshot of a nearby spiral galaxy called NGC 3175. NGC 3175 can be seen slicing across...

From a great distance, our Milky Way Galaxy would look like a thin disk of stars that orbits once every few hundred million years around its central region, where hundreds of billions of stars provide the gravitational ‘glue’ to hold it all together. But this pull of gravity is much weaker in the Galaxy’s far outer disk. There, the hydrogen atoms making up most of the Milky Way’s gas disk are no longer confined to a thin plane, instead they give the disk an S-like, or warped, appearance. Image credit: Xiaodian Chen.

Milky Way’s Thick Disk is 10 Billion Years Old, Astronomers Say

Dec 6, 2019 by News Staff

Our Milky Way Galaxy consists of two disk-like structures, known as ‘thick’ and ‘thin’ disks. The thick disk contains only about 20% of the Galaxy’s...

This composite image shows the surroundings of a supermassive black hole that is triggering star formation across the longest distance ever seen; as hot gas swirls around the black hole, it emits large amounts of X-rays that Chandra detects; the black hole is also the source of radio-wave emission from a jet of high-energy particles -- previously detected by scientists with the VLA -- that stretches about a million light-years. Image credit: NASA / CXC / INAF / R. Gilli et al / NRAO / VLA / STScI.

Supermassive Black Hole Triggers Star Formation in Multiple Galaxies

Dec 5, 2019 by News Staff

Enormous black holes usually affect their surroundings through the so-called ‘negative feedback’ — in other words, suppressing the formation...

This Hubble image shows the face-on spiral galaxy NGC 5468. The color image was made from separate exposures taken in the visible and infrared regions of the spectrum with Hubble’s Wide Field Camera 3 (WFC3). Four filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / W. Li et al / Judy Schmidt, www.geckzilla.com.

Hubble Space Telescope Observes NGC 5468

Dec 2, 2019 by News Staff

The NASA/ESA Hubble Space Telescope has produced a spectacularly detailed image of a spiral galaxy called NGC 5468. This Hubble image shows the face-on...

An artist’s impression of planets orbiting a supermassive black hole. Image credit: Kagoshima University.

Planets May Form and Orbit around Supermassive Black Holes

Nov 25, 2019 by Enrico de Lazaro

Protoplanetary disks around stars may not be the only site for planet formation in the Universe, according to a team of theoretical astrophysicists from...

This Hubble image shows the pair of interacting galaxies Arp 293. The image includes infrared observations from Hubble’s Wide Field Camera 3 (WFC3). Three filters were used to sample various wavelengths. Image credit: NASA / ESA / Hubble / K. Larson et al.

Hubble Witnesses Dance of Galaxies: Arp 293

Nov 25, 2019 by Natali Anderson

NASA has released a beautiful photo taken by the NASA/ESA Hubble Space Telescope of the peculiar pair of interacting galaxies called Arp 293. This Hubble...

This image of the Phoenix Cluster combines X-ray, radio and optical data; side panels show the individual images making up the composite. Image credit: NASA / CXC / MIT / M. McDonald et al / NRAO / AUI / NSF / STScI.

Enormous Black Hole Boosts Star Formation in Phoenix Galaxy Cluster

Nov 22, 2019 by News Staff

Supermassive black holes in the center of galaxy clusters usually suppress star formation, but the one in the Phoenix Cluster, a group of about 1,000 galaxies...

NGC 6240 harbors three supermassive black holes at its core: the northern black hole (N) is active and was known before; the zoomed-in new high-spatial resolution image shows that the southern component consists of two supermassive black holes (S1 and S2); the green color indicates the distribution of gas ionized by radiation surrounding the black holes; the red lines show the contours of the starlight from the galaxy and the length of the white bar corresponds to 1,000 light years. Image credit: P. Weilbacher, Leibniz Institute for Astrophysics Potsdam / NASA / ESA / Hubble Heritage / STScI / AURA / Hubble Collaboration / A. Evans, University of Virginia, Charlottesville / NRAO / Stony Brook University.

Astronomers Find Three Supermassive Black Holes in NGC 6240

Nov 22, 2019 by News Staff

NGC 6240, a well-studied nearby galaxy system in the process of merging, contains three supermassive black holes at its core, two of which are active and...

Astronomers Observe Host Galaxy of Extremely Bright and Long Gamma-Ray Burst

Nov 21, 2019 by News Staff

Astronomers have investigated the nature of a very bright and long-duration gamma-ray burst, GRB 190114C, by studying its environment. Hubble’s observations...

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