Tag Archive for 'Large Magellanic Cloud'

Left: this image from the Multi Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope shows the parent cloud LHA 120-N 180B in which the HH 1177 system was first observed. Center: this image shows the jets that accompany HH 1177; the top part of the jet is aimed slightly towards us and thus blueshifted; the bottom one is receding from us and thus redshifted. Right: this image from ALMA shows the rotating disk around the star, similarly with sides moving towards and away from us. Image credit: ESO / ALMA / NAOJ / NRAO / McLeod et al.

ALMA Spots Circumstellar Disk around Young Star in Large Magellanic Cloud

Nov 29, 2023 by News Staff

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have detected a rotating gaseous structure around an extragalactic massive young...

This image of SNR 1987A was taken with Webb’s Near-Infrared Camera. At the center, material ejected from the supernova forms a keyhole shape. Just to its left and right are faint crescents newly discovered by Webb. Beyond them an equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots. Exterior to that is diffuse emission and two faint outer rings. Image credit: NASA / ESA / CSA / M. Matsuura, Cardiff University / R. Arendt, NASA’s Goddard Spaceflight Center & University of Maryland, Baltimore County / C. Fransson.

Webb Focuses on Supernova 1987A Remnant

Aug 31, 2023 by Enrico de Lazaro

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have begun the study of SNR 1987A, one of the most renowned supernova remnants. This image...

This new Hubble image shows part of the Tarantula Nebula, which is located about 163,000 light-years away in the southern constellation of Dorado: wispy, nebulous clouds extend from the lower-left of the image; at the top and right the dark background of space can be seen through the sparse nebula; along the left and in the corner are many layers of brightly-colored gas and dark, obscuring dust; a cluster of small, bright blue stars in the same corner expands out across the image. Image credit: NASA / ESA / Hubble / C. Murray / E. Sabbi / Y.-H. Chu.

Hubble Space Telescope Focuses on Tarantula Nebula

Jan 30, 2023 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured a spectacular image of a very turbulent part of the Tarantula Nebula. This new Hubble...

This Hubble image shows the globular cluster NGC 1850, which is located in the Large Magellanic Cloud, over 160,000 light-years from Earth. For this image, five filters were used with the camera to gather data. Two of the filters were at near-ultraviolet wavelengths, two more at visible light wavelengths, and the final one was in the near-infrared. The data gathered through the two ultraviolet filters is violet and blue. The data from the two visible light filters is green and orange. The color red denotes near-infrared data. The image follows chromatic order, which means the shortest wavelength in the image is blue while the longest wavelength is red. Chromatic order allows us to visualize wavelengths of light beyond our eye’s sensitivity in a way that is familiar to us. Image credit: NASA / ESA / N. Bastian, Donostia International Physics Center / Gladys Kober, NASA & Catholic University of America.

Hubble Space Telescope Captures Dual Views of NGC 1850

Jan 3, 2023 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have taken two amazing images of NGC 1850, a young globular cluster located in the Large Magellanic...

This Hubble image shows NGC 2002, an open cluster some 160,000 light-years away in the southern constellation of Dorado. Image credit: NASA / ESA / G. Gilmore, University of Cambridge / Gladys Kober, NASA & Catholic University of America.

Hubble Captures Stunning View of NGC 2002

Dec 7, 2022 by Enrico de Lazaro

The Hubble team has released a beautiful new image of the open star cluster NGC 2002. This Hubble image shows NGC 2002, an open cluster some 160,000 light-years...

This Hubble image shows BSDL 2757, an open cluster some 160,000 light-years away in the constellation of Dorado. Image credit: NASA / ESA / L. Bianchi, Johns Hopkins University / G. Kober, NASA & Catholic University of America.

Hubble Sees Blue-White Stars in Distant Open Cluster

Dec 6, 2022 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured an amazing new photo of the open cluster BSDL 2757. This Hubble image shows BSDL 2757,...

This Hubble image shows DEM L 190, a young supernova remnant in the Large Magellanic Cloud. Image credit: NASA / ESA / Hubble / S. Kulkarni / Y. Chu.

Hubble Spots Colorful Supernova Remnant in Large Magellanic Cloud

Nov 28, 2022 by Enrico de Lazaro

The new Hubble image shows sheets and filaments of debris from a massive star that exploded as a supernova in the Large Magellanic Cloud, a nearby, small...

Shown here in purple, the Magellanic Corona stretches more than 100,000 light-years from the main mass of stars, gas, and dust that make up the Magellanic Clouds, intermingling with the hotter and more extensive corona that surrounds the Milky Way. Image credit: Leah Hustak, STScI.

Magellanic Corona: Astronomers Detect Protective Shield around Small and Large Magellanic Clouds

Oct 4, 2022 by News Staff

The Small and Large Magellanic Clouds — satellite galaxies of the Milky Way Galaxy — are surrounded by a diffuse halo of hot, supercharged...

This composite image shows SNR 0519-69.0, a Type Ia supernova remnant in the Large Magellanic Cloud: X-ray data from Chandra with low, medium and high energies are shown in green, blue, and purple respectively, with some of these colors overlapping to appear white; optical data from Hubble shows the perimeter of the remnant in red and stars around the remnant in white. Image credit: NASA / CXC / GSFC / Williams et al. / STScI.

Astronomers Determine Age of Supernova Remnant in Large Magellanic Cloud

Sep 14, 2022 by News Staff

Light from a Type Ia supernova explosion that created the supernova remnant SNR 0519-69.0 in the Large Magellanic Cloud, a satellite galaxy of the Milky...

This 340-light-year-wide image from Webb’s Near-Infrared Camera (NIRCam) shows the Tarantula Nebula. Image credit: NASA / ESA / CSA / STScI / Webb ERO Production Team.

Webb Takes Close Look at Tarantula Nebula

Sep 6, 2022 by News Staff

The Tarantula Nebula, a turbulent star-birth region located in the Large Magellanic Cloud, hosts thousands of young and still-forming stars, many revealed...

This image, taken with the Zorro imager on the 8.1-m Gemini South telescope, shows R136a1, the largest star yet discovered. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / T.A. Rector, University of Alaska Anchorage & NSF’s NOIRLab / M. Zamani, NSF’s NOIRLab / D. de Martin, NSF’s NOIRLab.

Gemini South Telescope Captures Best Ever Images of Most Massive Known Star

Aug 22, 2022 by Enrico de Lazaro

R136a1 has a mass between 170 and 230 solar masses, according to an analysis of optical data from the speckle imager Zorro mounted on the 8.1-m Gemini...

This artist’s impression shows what the binary system VFTS 243 might look like if we were observing it up close. The system, which is located in the Tarantula Nebula in the Large Magellanic Cloud, is composed of a hot, blue star with 25 times the Sun’s mass and a black hole, which is at least nine times the mass of the Sun. The sizes of the two binary components are not to scale: in reality, the blue star is about 200,000 times larger than the black hole. Image credit: ESO / L. Calçada.

Dormant Stellar-Mass Black Hole Detected in Tarantula Nebula

Jul 18, 2022 by News Staff

The newly-detected black hole is a member of the binary system VFTS 243, which is located in the famous Tarantula Nebula in the Large Magellanic Cloud. This...

This Hubble image shows the outskirts of the Tarantula Nebula. Image credit: NASA / ESA / Hubble / Josh Barrington.

Hubble Spots Glowing Plumes in Tarantula Nebula

Jun 30, 2022 by Enrico de Lazaro

NASA has released a beautiful photo taken by the Hubble Space Telescope of the outskirts of the Tarantula Nebula, which is located in the Large Magellanic...

This composite image shows the Tarantula Nebula. The background image, taken in the infrared, is itself a composite: it was captured by the HAWK-I instrument on ESO’s Very Large Telescope (VLT) and the Visible and Infrared Survey Telescope for Astronomy (VISTA), shows bright stars and light, pinkish clouds of hot gas. The bright red-yellow streaks that have been superimposed on the image come from radio observations taken by the ALMA, revealing regions of cold, dense gas which have the potential to collapse and form stars. The unique web-like structure of the gas clouds led astronomers to the nebula’s spidery nickname. Image credit: ESO / ALMA / NAOJ / NRAO / Wong et al. / M.-R. Cioni / VISTA Magellanic Cloud Survey / Cambridge Astronomical Survey Unit.

Astronomers Capture Spectacular Image of Tarantula Nebula

Jun 16, 2022 by News Staff

In a new high-resolution image, we see the Tarantula Nebula — a luminous star-forming region in the Large Magellanic Cloud, a satellite galaxy of...

These Spitzer and Webb images show part of the Large Magellanic Cloud. Image credit: NASA / JPL-Caltech / ESA / CSA / STScI.

Webb’s MIRI Camera Focuses on Large Magellanic Cloud

May 10, 2022 by News Staff

The NASA/ESA/CSA James Webb Space Telescope is aligned across all four of its science instruments, as seen in a previous engineering image. The Webb team...

This Hubble image shows DEM L 249, a remnant of Type Ia supernova located approximately 160,000 light-years away in the constellation of Mensa. Image credit: NASA / ESA / Hubble / Y. Chu.

Hubble Spots Tattered Remnant of Ancient Supernova in Large Magellanic Cloud

May 9, 2022 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope has captured a detailed image of a supernova remnant called DEM L 249. This Hubble image shows DEM L 249, a remnant...

A section of the Large Magellanic Cloud, captured under normal conditions by SARAO’s MeerKAT radio telescope. It is detecting all radio light, and PSR J0523-7125 looks like just another source of radio light. Image credit: Yuanming Wang.

ASKAP Radio Telescope Discovers New Extragalactic Pulsar

May 3, 2022 by News Staff

PSR J0523-7125, a highly circularly polarized, variable, steep-spectrum pulsar located in the Large Magellanic Cloud, is the brightest extragalactic pulsar...

The position of J0624-6948 (small object at the center of the purple ring indicated by *) is indicated with respect to the Milky Way’s Galactic plane, the Large Magellanic Cloud and the Small Magellanic Cloud. Image credit: Axel Mellinger, Central Michigan University.

ASKAP Finds Rogue Supernova Remnant near Large Magellanic Cloud

Mar 30, 2022 by News Staff

Astronomers using the Australian Square Kilometre Array Pathfinder (ASKAP) have spotted a mysterious circular ring between the Milky Way’s plane and...

This Hubble image shows NGC 1755, an open star cluster some 160,000 light-years away in the southern constellation of Dorado. The color image was made from separate exposures taken in the ultraviolet, visible and near-infrared regions of the spectrum with Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). 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 / A. Milone / G. Gilmore.

Hubble Spots Young Cluster in Large Magellanic Cloud

Dec 20, 2021 by Enrico de Lazaro

NASA has released a beautiful image snapped by the NASA/ESA Hubble Space Telescope of the open star cluster NGC 1755. This Hubble image shows NGC 1755,...

This artist’s impression shows NGC 1850 BH1 and a massive star orbiting it. The distortion of the star’s shape is due to the strong gravitational force exerted by the black hole. Image credit: M. Kornmesser / ESO.

Astronomers Detect Stellar-Mass Black Hole in Large Magellanic Cloud

Nov 12, 2021 by Natali Anderson

Astronomers using the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s Very Large Telescope have discovered a low-mass black hole in the...

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