Tag Archive for 'Supernova'

This Hubble image shows DEM L249, a remnant of Type Ia supernova located some 160,000 light-years away in the constellation of Mensa. Image credit: NASA / ESA / Hubble / Y. Chou, Institute of Astronomy and Astrophysics, Academia Sinica / Gladys Kober, NASA & Catholic University of America.

Hubble Observes Distant Remnant of Type Ia Supernova

Nov 9, 2021 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope shot this image of the supernova remnant DEM L249. This Hubble image shows DEM L249, a remnant of Type Ia supernova...

This Hubble image shows NGC 6984, a barred spiral galaxy some 164 million light-years away in the constellation of Indus. The color image is made up of observations from Hubble’s Wide Field Camera 3 (WFC3) in the ultraviolet, near-infrared, and optical parts of the spectrum. Six 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. Milisavljevic.

Hubble Sees Elegant Spiral Galaxy: NGC 6984

Nov 1, 2021 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured an amazing new photo of the barred spiral galaxy NGC 6984. This Hubble image shows...

False-color image of SN 2020fqv in its host galaxy system NGC 4567 and NGC 4568; the location of the supernova is shown in the inset. The image is composed of a pre-explosion single-band HST/WFPC2 image in the F606W filter with the color information from ground-based images obtained using the Nickel Telescope at Lick Observatory. The image of SN 2020fqv and the area outside of HST field of view is also from Nickel. Image credit: Joseph Depasquale / STScI.

Astronomers Observe ‘Rosetta Stone of Supernovae’

Oct 25, 2021 by News Staff

A Type II core-collapse supernova called SN 2020fqv exploded in NGC 4568, a member of a pair of colliding unbarred spiral galaxies; the other member of...

This composite image shows SNR G344.7-0.1 through the eyes of different telescopes: X-rays from Chandra (blue) have been combined with infrared data from NASA’s Spitzer Space Telescope (yellow and green) as well as radio data from the NSF’s Very Large Array and CSIRO’s Australia Telescope Compact Array (red). Image credit: NASA / CXC / Tokyo University of Science / Fukushima et al. / JPL / Spitzer / CSIRO / ATNF / ATCA.

Chandra Observes Distant Remnant of Type Ia Supernova

Oct 14, 2021 by News Staff

The Type Ia supernova remnant (SNR) G344.7-0.1 resides about 19,600 light-years away in the constellation of Scorpius. This composite image shows SNR G344.7-0.1...

This Hubble image shows the starburst spiral galaxy LEDA 42975. The color image was made from separate exposures taken in the visible and near-infrared regions of the spectrum with Hubble’s Wide Field Camera 3 (WFC3). It is based on data obtained through four filters. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / O. Graur / L. Shatz.

Hubble Looks at Stunning Starburst Spiral Galaxy

Oct 11, 2021 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured this vivid image of a spiral galaxy called LEDA 42975. This Hubble image shows the...

The location of the newly-discovered giant cavity within the Milky Way Galaxy is depicted on the right; a zoomed in view of the cavity (left) shows the Perseus and Taurus molecular clouds in blue and red, respectively; though they appear to sit within the cavity and touch, new 3D images of the clouds show they border the cavity and are quite a distance apart. Image credit: Alyssa Goodman / Harvard & Smithsonian Center for Astrophysics.

Astronomers Find Huge Spherical Cavity in Milky Way Galaxy

Sep 22, 2021 by News Staff

The 490-light-year-wide void is located among the constellations Perseus and Taurus, and was formed by one powerful supernova or a series of such events...

(a) WISE false color image of the Pa 30 nebula where blue and green stand for 11 μm emission, and red for 22 μm; (b) in this false color image, where green stands for WISE 11 μm (as in the left panel) and red for WISE 22 μm (adjusted to show extended emission), the emission from the central star is highlighted in blue from the GALEX near-UV data, while the XMM-Newton contors show that the majority of the X-ray emission originates from the core of the nebula; a background point source is seen westward of the CS in the XMM-Newton contour map; (c) the 2.1 m KPNO image; the green cross in the center of the image marks the location of the CS; panels (a)-(c) are reproduced at the same angular scale and orientation; at the Gaia distance of Pa 30 of 2,300 parsecs, an angular scale of 45'' translates to about 100,000 AU. Image credit: Ritter et al., doi: 10.3847/2041-8213/ac2253.

Astronomers Identify Remnant of Historical Supernova SN 1181

Sep 20, 2021 by News Staff

New research led by University of Hong Kong astronomers shows that a fast expanding nebula called Pa 30 surrounding the hot Wolf-Rayet star IRAS 00500+6713...

Fast-moving debris from a supernova explosion triggered by a stellar collision in the VT 1210+4956 system crashes into material thrown out earlier, and the shocks cause bright radio emission seen by the VLA. Image credit: Bill Saxton / NRAO / AUI / NSF.

Compact Object Collision with Companion Star Triggers Supernova Event

Sep 2, 2021 by News Staff

Using data collected by the Very Large Array Sky Survey (VLASS), astronomers have found evidence that a compact object — a black hole or neutron...

Multi-wavelength observations of the Ophiuchus star-forming region reveal interactions between clouds of star-forming gas and radionuclides produced in a nearby cluster of young stars. The top image (a) shows the distribution of aluminum-26 in red, traced by gamma-ray emissions. The central box represents the area covered in the bottom left image (b), which shows the distribution of protostars in the Ophiuchus clouds as red dots. The area in the box is shown in the bottom right image (c), a deep near-infrared color composite image of the L1688 cloud, containing many well known prestellar dense-gas cores with disks and protostars. Image credit: Forbes et al., doi: 10.1038/s41550-021-01442-9.

Ophiuchus Star-Forming Complex Hosts Analogues of Early Solar System, Astronomers Say

Aug 17, 2021 by News Staff

The Ophiuchus star-forming complex is a complex of interstellar clouds, nebulae and prestellar cores in the constellation of Ophiuchus. At an estimated...

This image shows galaxy Arp 148, captured by NASA’s Spitzer Space Telescope and the NASA/ESA Hubble Space Telescope; specially processed Spitzer data is shown inside the white circle, revealing infrared light from a supernova hidden by dust; this is one five hidden supernovae documented by Fox et al. Image credit: NASA / JPL-Caltech.

Spitzer Discovers Five Dust-Obscured Supernovae

Aug 4, 2021 by News Staff

Astronomers using data from NASA’s Spitzer Space Telescope have looked for dust-extinguished supernovae in the nuclear regions of 40 luminous and ultra-luminous...

An artist’s impression of a thermonuclear supernova event. Image credit: ESA / ATG Medialab / C. Carreau.

Astronomers Spot Spinning Runaway Star

Aug 4, 2021 by News Staff

Using the NASA/ESA Hubble Space Telescope and NASA’s Transiting Exoplanet Survey Satellite (TESS), astronomers have detected 8.9-hr variability in both...

This illustration depicts a collapsing star that is producing two short gamma-ray jets. Image credit: Gemini Observatory / NOIRLab / NSF / AURA / J. da Silva / M. Zamani, NOIRLab.

Shortest Supernova-Produced Gamma-Ray Burst Discovered

Jul 28, 2021 by News Staff

Most known supernova-powered gamma-ray bursts are ‘long’ (lasting more than two seconds), but a gamma-ray burst event called GRB 200826A lasted just...

This Hubble image shows the galaxy cluster MACS J0138.0-2155, which is so massive that its gravity bent and magnified light streaming not only from an extremely distant background galaxy but also from a supernova event in this galaxy. The color image was made using observations from eight different filters spread across Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / A. Newman / M. Akhshik / K. Whitaker.

Hubble Observes Multiply-Imaged, Gravitationally Lensed Supernova

Jul 19, 2021 by Enrico de Lazaro

The multiply-imaged supernova AT2016jka appeared in the distant giant galaxy MRG-M0138, gravitationally lensed by the foreground galaxy cluster MACS J0138.0-2155. This...

An artist’s impression of HD 265435, a binary system located approximately 1,500 light-years away in the constellation of Gemini. Image credit: Mark Garlick / University of Warwick.

HD 265435 Will Explode as Type Ia Supernova in 70 Million Years, Astronomers Say

Jul 13, 2021 by News Staff

HD 265435 is a binary system with an orbital period of around 100 min that consists of a white dwarf and a hot subdwarf star. An artist’s impression...

Las Cumbres/Hubble composite image of the electron-capture supernova SN 2018zd (the large white dot on the right) and the host starburst galaxy NGC 2146 (toward the left). Image credit: NASA / ESA / Hubble / STScI / J. DePasquale, Las Cumbres Observatory.

Astronomers Discover Third Type of Supernova

Jun 29, 2021 by News Staff

An international team of astronomers has discovered the first convincing evidence for an electron-capture supernova, which is thought to arise from the...

This image from NASA’s Chandra X-ray Observatory shows the supernova remnant MSH 15-52. Image credit: NASA / SAO / NCSU / Borkowski et al.

NASA’s Chandra X-ray Observatory Watches Fast Blast Wave from Exploded Star

Jun 25, 2021 by News Staff

A stellar structure known as the ‘Hand of God’ is a nebula of energy and particles blown by a pulsar left behind after a star exploded in our Milky...

This composite image, taken by NASA’s Chandra X-ray Observatory and the NASA/ESA Hubble Space Telescope, shows the supernova remnant Cassiopeia A; the different colors represent elements detected by Chandra: iron (orange), oxygen (purple), and the amount of silicon compared to magnesium (green); titanium (light blue) detected previously by NASA’s NuSTAR telescope is shown, but not the different type of titanium found by Chandra. Image credit: NASA / CXC / RIKEN / Sato et al. / NuSTAR.

Chandra Detects Stable Isotope of Titanium in Cassiopeia A

Apr 28, 2021 by News Staff

Astronomers using NASA’s Chandra X-ray Observatory have detected stable titanium, along with chromium and iron, blasting out from the center of the supernova...

This image from the SRG/eROSITA all-sky survey shows SNR Hoinga (marked); the large bright source in the lower quadrant of the image is from SNR Vela; the image colors are correlated with the energies of the detected X-ray photons; red represents the 0.3-0.6 keV energy range, green 0.6-1.0 keV and blue 1.0-2.3 keV. Image credit: SRG / eROSITA / Becker et al., doi: 10.1051/0004-6361/202040156.

eROSITA X-Ray Telescope Spots Enormous Supernova Remnant

Mar 5, 2021 by News Staff

Astronomers using data from the eROSITA X-ray telescope aboard the Spektrum-Roentgen-Gamma (SRG) observatory have detected the largest supernova remnant...

SN 1987A: the panel on the left contains a 3D computer simulation, based on Chandra data, of the supernova debris from SN 1987A crashing into a surrounding ring of material; the artist’s illustration (right panel) depicts a so-called pulsar wind nebula, a web of particles and energy blown away from a pulsar, which is a rotating, highly magnetized neutron star. Image credit: NASA / Chandra / CXC / University di Palermo / E. Greco / INAF-Osservatorio Astronomico di Palermo / Salvatore Orlando.

Astronomers Finally Find Neutron Star in Famous Supernova Remnant

Feb 26, 2021 by News Staff

Supernova 1987A (SN 1987A) was first observed on February 23, 1987 in a nearby dwarf galaxy, the Large Magellanic Cloud, some 164,000 light-years away....

3D reconstruction of the Crab Nebula remnant as seen from Earth (left), and from another point of view showing its heart-shaped morphology (right). Image credit: Martin et al., doi: 10.1093/mnras/staa4046.

Crab Nebula Has ‘Honeycomb Heart,’ Astronomers Say

Feb 18, 2021 by News Staff

New images captured by the SITELLE instrument on the Canada-France-Hawaii telescope (CFHT) in Mauna Kea, Hawaii, reveal an intricate honeycomb-like arrangement...

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