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VizieR J/A+A/707/A50

New in the #VirtualObservatory: “Massive runaway star HD 254577” by Dincel B. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A50
#SupernovaRemnants #Spectroscopy #VisibleAstronomy

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Information on resource 'Northern Sky Narrowband Survey: Continuum HIPS'

New in the #VirtualObservatory: “Northern Sky Narrowband Survey: Continuum HIPS” by Ziegenbalg, S.
http://dc.g-vo.org/browse/nsns/cont
#EmissionNebulae #SupernovaRemnants #Ism #SkySurveys

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VizieR J/A+A/701/A206

New in the #VirtualObservatory: “Puppis A Fermi-LAT TS and eROSITA images” by Giuffrida R. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/701/A2...
#GammaRayAstronomy #SupernovaRemnants #RadioSources

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VizieR J/ApJ/949/74

New in the #VirtualObservatory: “Spitzer, WISE & Herschel obs. of the young SNR N132D” by Rho J. et al.
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/949/74
#SupernovaRemnants #InfraredAstronomy #Spectroscopy #MagellanicClouds

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Information on resource 'Northern Sky Narrowband Survey'

New in the #VirtualObservatory: “Northern Sky Narrowband Survey” by Ziegenbalg, S.
http://dc.g-vo.org/browse/nsns/q
#Ism #SupernovaRemnants #PlanetaryNebulae #EmissionNebulae

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VizieR J/A+A/700/A223

New in the #VirtualObservatory: “Discovery of seven extragalactic O-rich SNRs” by Kravtsov T. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/700/A2...
#Spectroscopy #SupernovaRemnants #Galaxies

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VizieR J/A+A/699/A319

New in the #VirtualObservatory: “EVLA and LOFAR images of Crab Nebula” by Arias M. et al.
cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/A3...
#SupernovaRemnants #RadioSources

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A high-resolution radio image of the Milky Way's galactic center, revealing intricate structures like arcs, threads, and supernova remnants.  The bright region, Sagittarius A*, is suspected to harbor a supermassive black hole. This image from the Very Large Array showcases the dynamic and enigmatic nature of our galaxy's core.

A high-resolution radio image of the Milky Way's galactic center, revealing intricate structures like arcs, threads, and supernova remnants. The bright region, Sagittarius A*, is suspected to harbor a supermassive black hole. This image from the Very Large Array showcases the dynamic and enigmatic nature of our galaxy's core.

Astronomy Picture from 03/08/2002

The Galactic Center - A Radio Mystery

Source: https://apod.nasa.gov/apod/ap020803.html


#MilkyWayCenter #GalacticCenter #RadioAstronomy #VLA #BlackHole #SupernovaRemnants #CosmicThreads #Astrophysics #SpaceExploration #AstronomyImage #SagittariusA #DeepSpace

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Adding Dimension to Cassiopeia A Using NASA’s James Webb Space Telescope, astronomers uncovered a mysterious feature within the remnant, nicknamed the “Green Monster,” alongside a puzzling network of ejecta filaments forming a web of oxygen-rich material. When combined with X-rays from NASA’s Chandra X-ray Observatory, the data helped astronomers shed light on the origin of the Green Monster and revealed […] The post Adding Dimension to Cassiopeia A first appeared on VibeWire Magazine.

#SupernovaRemnants

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Seeing the Cygnus Loop in a New Way The Cygnus Loop, also known as the Veil Nebula, is a supernova remnant – the remains of the explosive death of a massive star. Studying images like these leads to discovery, but NASA’s Chandra X-ray Observatory provides another way to experience this data: three-dimensional (3D) models that allow people to explore – and print – […] The post Seeing the Cygnus Loop in a New Way first appeared on VibeWire Magazine.

#SupernovaRemnants

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Chandra X-ray Observatory image of M82 (the Cigar Galaxy), showcasing a vibrant, crimson nebula filled with bright spots – likely shocked supernova remnants and X-ray bright binary stars.  This starburst galaxy exhibits a remarkably high rate of star formation, fueled by galactic interactions and displaying the dramatic effects of stellar winds and supernova explosions.

Chandra X-ray Observatory image of M82 (the Cigar Galaxy), showcasing a vibrant, crimson nebula filled with bright spots – likely shocked supernova remnants and X-ray bright binary stars. This starburst galaxy exhibits a remarkably high rate of star formation, fueled by galactic interactions and displaying the dramatic effects of stellar winds and supernova explosions.

Astronomy Picture from 21/04/2000

M82: Starburst In X-rays

Source: https://apod.nasa.gov/apod/ap000421.html


#StarburstGalaxy #M82 #CigarGalaxy #ChandraXray #SupernovaRemnants #Space #Astronomy #Astrophysics #Galaxy #StarFormation #Cosmology

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Infrared image of galactic dust clouds in the Cygnus region of the Milky Way. The dust is arranged in a foam-like structure with bubbles and voids, likely formed by stellar winds and supernovae shocks.  The image reveals bright, bubble-shaped, and arc-like clouds around supernova remnants and star-forming regions.  Data from NASA's IRAS satellite.

Infrared image of galactic dust clouds in the Cygnus region of the Milky Way. The dust is arranged in a foam-like structure with bubbles and voids, likely formed by stellar winds and supernovae shocks. The image reveals bright, bubble-shaped, and arc-like clouds around supernova remnants and star-forming regions. Data from NASA's IRAS satellite.

Astronomy Picture from 24/04/1997

The Frothy Milky Way
Credit:

Source: https://apod.nasa.gov/apod/ap970424.html


#MilkyWay #CosmicFoam #GalacticDust #IRAS #Astrophysics #SpaceScience #StarBirth #SupernovaRemnants #AstronomyPictureOfTheDay #NASA

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Infrared image of the Milky Way's galactic plane near Cygnus, revealing a frothy texture of dust clouds.  Bright, bubble-shaped and arc-like structures are visible around supernova remnants and star-forming regions. The image, based on data from NASA's IRAS satellite, shows the complex distribution of dust, resembling a foamy glass of beer.

Infrared image of the Milky Way's galactic plane near Cygnus, revealing a frothy texture of dust clouds. Bright, bubble-shaped and arc-like structures are visible around supernova remnants and star-forming regions. The image, based on data from NASA's IRAS satellite, shows the complex distribution of dust, resembling a foamy glass of beer.

Astronomy Picture from 24/04/1997

The Frothy Milky Way
Credit:

Source: https://apod.nasa.gov/apod/ap970424.html


#MilkyWayFoam #GalacticDust #CosmicBubbles #IRASData #StarBirth #SupernovaRemnants #Astrophysics #SpaceScience #AstronomyImage #NASA

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A stunning Hubble Space Telescope image of NGC 1850, a unique double star cluster in the Large Magellanic Cloud.  The larger cluster contains stars around 50 million years old, while the smaller cluster boasts even younger stars, approximately 4 million years old.  Glowing gas filaments, remnants of supernova explosions, are also visible, highlighting the region's dynamic stellar activity. This cluster is unlike anything found in our Milky Way galaxy.

A stunning Hubble Space Telescope image of NGC 1850, a unique double star cluster in the Large Magellanic Cloud. The larger cluster contains stars around 50 million years old, while the smaller cluster boasts even younger stars, approximately 4 million years old. Glowing gas filaments, remnants of supernova explosions, are also visible, highlighting the region's dynamic stellar activity. This cluster is unlike anything found in our Milky Way galaxy.

Astronomy Picture from 20/02/2023

NGC 1850: Not Found in the Milky Way

Source: https://apod.nasa.gov/apod/ap230220.html


#HubbleSpaceTelescope #NGC1850 #StarCluster #LargeMagellanicCloud #Astronomy #Space #Cosmology #Stars #Nebula #DoubleStarCluster #MilkyWay #YoungStars #SupernovaRemnants

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Four panels showcasing x-ray images of supernova remnants (SNRs) in the Large Magellanic Cloud.  Clockwise from top left, the SNRs depict ages of 600, 1500, 10,000, and 13,000 years, illustrating the expansion of cosmic debris from stellar explosions (Type Ia & Type II).  The lower left SNR shows a neutron star at its center.

Four panels showcasing x-ray images of supernova remnants (SNRs) in the Large Magellanic Cloud. Clockwise from top left, the SNRs depict ages of 600, 1500, 10,000, and 13,000 years, illustrating the expansion of cosmic debris from stellar explosions (Type Ia & Type II). The lower left SNR shows a neutron star at its center.

Astronomy Picture from 28/07/2006

Four Supernova Remnants

Source: https://apod.nasa.gov/apod/ap060728.html


#SupernovaRemnants #CosmicDebris #LargeMagellanicCloud #XRayAstronomy #StellarExplosions #TypeIa #TypeII #NeutronStar #AstronomyImage #SpaceScience

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A true-color image of M81, showcasing a nebula spanning 300 light-years.  The image highlights the homes of young stars and the remnants of two exploded stars within the nebula's vibrant, swirling structure.  The colors reveal the complex processes of stellar birth and death within this cosmic region.

A true-color image of M81, showcasing a nebula spanning 300 light-years. The image highlights the homes of young stars and the remnants of two exploded stars within the nebula's vibrant, swirling structure. The colors reveal the complex processes of stellar birth and death within this cosmic region.

Astronomy Picture from 25/07/1997

Stellar Laboratories in the LMC

Source: https://apod.nasa.gov/apod/ap970725.html


#M81 #TrueColor #Nebula #StarBirth #SupernovaRemnants #Space #Astronomy #Astrophysics #Cosmos #DeepSpace #Galaxy #StarClusters #StellarEvolution

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Check out this breathtaking Southern #SeagullNebula Complex by Team #Celestron @dylanodonnell w/ his #C11 #EdgeHD.

This region is packed with man celestial objects including emission & reflection #nebulae, #supernovaremnants, #starclusters, star-forming regions, & a #Wolf-Rayet.

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Bat Nebula (NGC 6995)

The Bat Nebula, located around 2,400 light-years away in the Cygnus constellation, resembles a bat with its wings spread. It‘s part of the larger Veil Nebula, formed by a supernova explosion.

#BatNebula #VeilNebula #AstronomyLovers #CosmicWonders #SupernovaRemnants

Bat Nebula (NGC 6995) The Bat Nebula, located around 2,400 light-years away in the Cygnus constellation, resembles a bat with its wings spread. It‘s part of the larger Veil Nebula, formed by a supernova explosion. #BatNebula #VeilNebula #AstronomyLovers #CosmicWonders #SupernovaRemnants

Bat Nebula (NGC 6995)

The Bat Nebula, located around 2,400 light-years away in the Cygnus constellation, resembles a bat with its wings spread. It‘s part of the larger Veil Nebula, formed by a supernova explosion.

#BatNebula #VeilNebula #AstronomyLovers #CosmicWonders #SupernovaRemnants

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