#seyfert — Public Fediverse posts
Live and recent posts from across the Fediverse tagged #seyfert, aggregated by home.social.
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UGC 11397 is a barred spiral galaxy located in the constellation Lyra . It is notable for being classified as a Type 2 #Seyfert galaxy, which is a type of active galaxy.
Its center is highly energetic (an active galactic nucleus) but the activity is largely obscured from view in visible light by a thick, donut-shaped cloud of dust and gas.
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UGC 11397 is a barred spiral galaxy located in the constellation Lyra . It is notable for being classified as a Type 2 #Seyfert galaxy, which is a type of active galaxy.
Its center is highly energetic (an active galactic nucleus) but the activity is largely obscured from view in visible light by a thick, donut-shaped cloud of dust and gas.
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UGC 11397 is a barred spiral galaxy located in the constellation Lyra . It is notable for being classified as a Type 2 #Seyfert galaxy, which is a type of active galaxy.
Its center is highly energetic (an active galactic nucleus) but the activity is largely obscured from view in visible light by a thick, donut-shaped cloud of dust and gas.
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UGC 11397 is a barred spiral galaxy located in the constellation Lyra . It is notable for being classified as a Type 2 #Seyfert galaxy, which is a type of active galaxy.
Its center is highly energetic (an active galactic nucleus) but the activity is largely obscured from view in visible light by a thick, donut-shaped cloud of dust and gas.
-
UGC 11397 is a barred spiral galaxy located in the constellation Lyra . It is notable for being classified as a Type 2 #Seyfert galaxy, which is a type of active galaxy.
Its center is highly energetic (an active galactic nucleus) but the activity is largely obscured from view in visible light by a thick, donut-shaped cloud of dust and gas.
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#Seyfert galaxies are characterized by an extremely active galactic nucleus (AGN) where a supermassive black hole is actively consuming matter and emitting enormous amounts of radiation.
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#Seyfert galaxies are characterized by an extremely active galactic nucleus (AGN) where a supermassive black hole is actively consuming matter and emitting enormous amounts of radiation.
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#Seyfert galaxies are characterized by an extremely active galactic nucleus (AGN) where a supermassive black hole is actively consuming matter and emitting enormous amounts of radiation.
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#Seyfert galaxies are characterized by an extremely active galactic nucleus (AGN) where a supermassive black hole is actively consuming matter and emitting enormous amounts of radiation.
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#Seyfert galaxies are characterized by an extremely active galactic nucleus (AGN) where a supermassive black hole is actively consuming matter and emitting enormous amounts of radiation.
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#Seyfert galaxies are a class of active galaxies that have very bright centers. They are named after American astronomer Carl Seyfert, who first observed them in 1943.
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#Seyfert galaxies are a class of active galaxies that have very bright centers. They are named after American astronomer Carl Seyfert, who first observed them in 1943.
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#Seyfert galaxies are a class of active galaxies that have very bright centers. They are named after American astronomer Carl Seyfert, who first observed them in 1943.
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#Seyfert galaxies are a class of active galaxies that have very bright centers. They are named after American astronomer Carl Seyfert, who first observed them in 1943.
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#Seyfert galaxies are a class of active galaxies that have very bright centers. They are named after American astronomer Carl Seyfert, who first observed them in 1943.
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De Hubble Space Telescope werpt een blik op UGC 3478
Een schitterende nieuwe afbeelding, gemaakt door de Hubble Space Telescope, biedt een gedetailleerde blik op het spiraalstelsel UGC 3478.
https://www.kuuke.nl/de-hubble-space-telescope-werpt-een-blik-op-ugc-3478/
#camelopardalis #giraffe #hubble #seyfert #seyfertstelsel #sterrenbeeld #UGC3478 #ZwartGat
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Bildveröffentlichung / #Hubble: Die #Spiralgalaxie NGC 4951
https://www.astropage.eu/2024/07/02/bildveroeffentlichung-hubble-die-spiralgalaxie-ngc-4951/
#Weltraumteleskop, #Galaxie, #Sternentstehung, #Seyfert-Galaxie
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#MartinSeyfert 16?? — 1744
#OboeConcerto in C minor :
I. Allegro
II. Largo
III. Allegro#HansHeinrichKriegel #Oboe
#CatervaMusica#musik #music #musique #musica #classicalmusic #Seyfert #Galantmusic
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#MartinSeyfert 16?? — 1744
#OboeConcerto in C minor :
I. Allegro
II. Largo
III. Allegro#HansHeinrichKriegel #Oboe
#CatervaMusica#musik #music #musique #musica #classicalmusic #Seyfert #Galantmusic
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#MartinSeyfert 16?? — 1744
#OboeConcerto in C minor :
I. Allegro
II. Largo
III. Allegro#HansHeinrichKriegel #Oboe
#CatervaMusica#musik #music #musique #musica #classicalmusic #Seyfert #Galantmusic
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#MartinSeyfert 16?? — 1744
#OboeConcerto in C minor :
I. Allegro
II. Largo
III. Allegro#HansHeinrichKriegel #Oboe
#CatervaMusica#musik #music #musique #musica #classicalmusic #Seyfert #Galantmusic
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#MartinSeyfert 16?? — 1744
#OboeConcerto in C minor :
I. Allegro
II. Largo
III. Allegro#HansHeinrichKriegel #Oboe
#CatervaMusica#musik #music #musique #musica #classicalmusic #Seyfert #Galantmusic
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Hubble fotografeert het balkspiraalstelsel NGC 3783
Astronomen hebben de Hubble Space Telescope gebruikt om een opname te maken van het heldere balkspiraalstelsel NGC 34783. NGC 3783 bevindt zich op een afstand van ongeveer 135 miljoen lichtjaar in de richting van het sterrenbeeld Centaurus.
https://www.kuuke.nl/hubble-fotografeert-het-balkspiraalstelsel-ngc-3783/
#balkspiraalstelsel #centaurus #hubble #NGC3783 #seyfert #sterrenstelsel
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XMM-Newton detecteert ultrasnelle zwartegatwind in Markarian 817
Markarian 817 is een Seyfert 1-sterrenstelsel dat ongeveer 430 miljoen lichtjaar van ons is verwijderd in de richting van het sterrenbeeld Draco – Draak. Het bevat een supermassief zwart gat met een massa van 81 miljoen zonsmassa.
https://www.kuuke.nl/xmm-newton-detecteert-ultrasnelle-zwartegatwind-in-markarian-817/
#esa #Markarian817 #rntgenstraling #seyfert #XMMNewton #ZwartGat #zwartwgatwind
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¡#HolaCiencia! MCG-01-24-014 es una #galaxia espiral #Seyfert de tipo-2 que emite luz teóricamente "prohibida" en condiciones de laboratorio, pero que aparece con las altísimas energías presentes en el seno de su núcleo activo • #FotoCiencia ESA/Hubble, NASA, C. Kilpatrick
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¡#HolaCiencia! MCG-01-24-014 es una #galaxia espiral #Seyfert de tipo-2 que emite luz teóricamente "prohibida" en condiciones de laboratorio, pero que aparece con las altísimas energías presentes en el seno de su núcleo activo • #FotoCiencia ESA/Hubble, NASA, C. Kilpatrick
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¡#HolaCiencia! MCG-01-24-014 es una #galaxia espiral #Seyfert de tipo-2 que emite luz teóricamente "prohibida" en condiciones de laboratorio, pero que aparece con las altísimas energías presentes en el seno de su núcleo activo • #FotoCiencia ESA/Hubble, NASA, C. Kilpatrick
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¡#HolaCiencia! MCG-01-24-014 es una #galaxia espiral #Seyfert de tipo-2 que emite luz teóricamente "prohibida" en condiciones de laboratorio, pero que aparece con las altísimas energías presentes en el seno de su núcleo activo • #FotoCiencia ESA/Hubble, NASA, C. Kilpatrick
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¡#HolaCiencia! MCG-01-24-014 es una #galaxia espiral #Seyfert de tipo-2 que emite luz teóricamente "prohibida" en condiciones de laboratorio, pero que aparece con las altísimas energías presentes en el seno de su núcleo activo • #FotoCiencia ESA/Hubble, NASA, C. Kilpatrick
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The Point Spread Function of the James #Webb Space Telescope is severe and in particular images with MIRI are affected - but now the paper "Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728" (https://arxiv.org/abs/2312.14307) offers a way out: here is a #Seyfert galaxy image before and after running it though the #Kraken algorithm.
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The Point Spread Function of the James #Webb Space Telescope is severe and in particular images with MIRI are affected - but now the paper "Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728" (https://arxiv.org/abs/2312.14307) offers a way out: here is a #Seyfert galaxy image before and after running it though the #Kraken algorithm.
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The Point Spread Function of the James #Webb Space Telescope is severe and in particular images with MIRI are affected - but now the paper "Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728" (https://arxiv.org/abs/2312.14307) offers a way out: here is a #Seyfert galaxy image before and after running it though the #Kraken algorithm.
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The Point Spread Function of the James #Webb Space Telescope is severe and in particular images with MIRI are affected - but now the paper "Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728" (https://arxiv.org/abs/2312.14307) offers a way out: here is a #Seyfert galaxy image before and after running it though the #Kraken algorithm.
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The Point Spread Function of the James #Webb Space Telescope is severe and in particular images with MIRI are affected - but now the paper "Deconvolution of JWST/MIRI Images: Applications to an AGN Model and GATOS Observations of NGC 5728" (https://arxiv.org/abs/2312.14307) offers a way out: here is a #Seyfert galaxy image before and after running it though the #Kraken algorithm.
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Bildveröffentlichung / #Hubble: Die #Seyfert-#Galaxie MCG-01-24-014
https://www.astropage.eu/2023/12/19/bildveroeffentlichung-hubble-die-seyfert-galaxie-mcg-01-24-014/
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X-ray emission from a rapidly accreting narrow-line #Seyfert 1 galaxy at z = 6.56: https://www.aanda.org/articles/aa/full_html/2023/01/aa44688-22/aa44688-22.html -> Serendipitous detection of a rapidly accreting #blackhole in the early Universe - #eROSITA telescope finds an X-ray bright, optically faint quasar accreting material at an extremely high rate only about 800 million years after the big bang: https://www.mpe.mpg.de/7925669/news20230131
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X-ray emission from a rapidly accreting narrow-line #Seyfert 1 galaxy at z = 6.56: https://www.aanda.org/articles/aa/full_html/2023/01/aa44688-22/aa44688-22.html -> Serendipitous detection of a rapidly accreting #blackhole in the early Universe - #eROSITA telescope finds an X-ray bright, optically faint quasar accreting material at an extremely high rate only about 800 million years after the big bang: https://www.mpe.mpg.de/7925669/news20230131
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X-ray emission from a rapidly accreting narrow-line #Seyfert 1 galaxy at z = 6.56: https://www.aanda.org/articles/aa/full_html/2023/01/aa44688-22/aa44688-22.html -> Serendipitous detection of a rapidly accreting #blackhole in the early Universe - #eROSITA telescope finds an X-ray bright, optically faint quasar accreting material at an extremely high rate only about 800 million years after the big bang: https://www.mpe.mpg.de/7925669/news20230131
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X-ray emission from a rapidly accreting narrow-line #Seyfert 1 galaxy at z = 6.56: https://www.aanda.org/articles/aa/full_html/2023/01/aa44688-22/aa44688-22.html -> Serendipitous detection of a rapidly accreting #blackhole in the early Universe - #eROSITA telescope finds an X-ray bright, optically faint quasar accreting material at an extremely high rate only about 800 million years after the big bang: https://www.mpe.mpg.de/7925669/news20230131
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X-ray emission from a rapidly accreting narrow-line #Seyfert 1 galaxy at z = 6.56: https://www.aanda.org/articles/aa/full_html/2023/01/aa44688-22/aa44688-22.html -> Serendipitous detection of a rapidly accreting #blackhole in the early Universe - #eROSITA telescope finds an X-ray bright, optically faint quasar accreting material at an extremely high rate only about 800 million years after the big bang: https://www.mpe.mpg.de/7925669/news20230131
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Another one of our #jwstgoals #ers1328 galaxies -- #NGC7469 -- is now featured on the ESA blog as Picture of the Month 🤩
See Armus+22 for the detailed AGN spectrum; U+22 for the AGN outflow, Lai+22 for the dust grain sizes, and Bohn+22 for the young stars in the ring!
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Another one of our #jwstgoals #ers1328 galaxies -- #NGC7469 -- is now featured on the ESA blog as Picture of the Month 🤩
See Armus+22 for the detailed AGN spectrum; U+22 for the AGN outflow, Lai+22 for the dust grain sizes, and Bohn+22 for the young stars in the ring!
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Another one of our #jwstgoals #ers1328 galaxies -- #NGC7469 -- is now featured on the ESA blog as Picture of the Month 🤩
See Armus+22 for the detailed AGN spectrum; U+22 for the AGN outflow, Lai+22 for the dust grain sizes, and Bohn+22 for the young stars in the ring!
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Another one of our #jwstgoals #ers1328 galaxies -- #NGC7469 -- is now featured on the ESA blog as Picture of the Month 🤩
See Armus+22 for the detailed AGN spectrum; U+22 for the AGN outflow, Lai+22 for the dust grain sizes, and Bohn+22 for the young stars in the ring!