#headerpicture — Public Fediverse posts
Live and recent posts from across the Fediverse tagged #headerpicture, aggregated by home.social.
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✨ New header picture 🖼️
The image shows the numerical simulation results of a binary black hole merger consistent with the gravitational-wave event GW231123.
GW231123 was recently announced as the merger of the most massive black holes ever observed with gravitational waves. Models that account for the complex dynamics of highly spinning black holes, which were developed at the @mpi_grav, were used to analyze the signal and extract astrophysical information from it.
The image is by I. Markin (@unipotsdam), H. Pfeiffer (@mpi_grav), T. Dietrich (@unipotsdam and @mpi_grav)
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✨ New header picture 🖼️
The image shows the numerical simulation results of a binary black hole merger consistent with the gravitational-wave event GW231123.
GW231123 was recently announced as the merger of the most massive black holes ever observed with gravitational waves. Models that account for the complex dynamics of highly spinning black holes, which were developed at the @mpi_grav, were used to analyze the signal and extract astrophysical information from it.
The image is by I. Markin (@unipotsdam), H. Pfeiffer (@mpi_grav), T. Dietrich (@unipotsdam and @mpi_grav)
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✨ New header picture 🖼️
The image shows the numerical simulation results of a binary black hole merger consistent with the gravitational-wave event GW231123.
GW231123 was recently announced as the merger of the most massive black holes ever observed with gravitational waves. Models that account for the complex dynamics of highly spinning black holes, which were developed at the @mpi_grav, were used to analyze the signal and extract astrophysical information from it.
The image is by I. Markin (@unipotsdam), H. Pfeiffer (@mpi_grav), T. Dietrich (@unipotsdam and @mpi_grav)
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✨ New header picture 🖼️
The image shows the numerical simulation results of a binary black hole merger consistent with the gravitational-wave event GW231123.
GW231123 was recently announced as the merger of the most massive black holes ever observed with gravitational waves. Models that account for the complex dynamics of highly spinning black holes, which were developed at the @mpi_grav, were used to analyze the signal and extract astrophysical information from it.
The image is by I. Markin (@unipotsdam), H. Pfeiffer (@mpi_grav), T. Dietrich (@unipotsdam and @mpi_grav)
-
✨ New header picture 🖼️
The image shows the numerical simulation results of a binary black hole merger consistent with the gravitational-wave event GW231123.
GW231123 was recently announced as the merger of the most massive black holes ever observed with gravitational waves. Models that account for the complex dynamics of highly spinning black holes, which were developed at the @mpi_grav, were used to analyze the signal and extract astrophysical information from it.
The image is by I. Markin (@unipotsdam), H. Pfeiffer (@mpi_grav), T. Dietrich (@unipotsdam and @mpi_grav)
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🚨 New header picture 🖼️
Researchers from the independent @maxplanckgesellschaft research group “Binary Merger Observations and Numerical Relativity” have studied how the spins of merging black holes influence the recoil after their merger, and how this in turn influences the remnant spin magnitudes after repeated mergers in dense stellar environments.
The header picture shows some of their results.
ℹ️ https://www.aei.mpg.de/1244528/towards-a-deeper-understanding-of-black-hole-origins?c=785562
📄 https://arxiv.org/abs/2503.21278 (The header picture is Fig. 5 in there)
#HeaderPicture #BlackHoles #BlackHoleKicks #BlackHoleWeek #Astrodon #Astronomy
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🚨 New header picture 🖼️
Researchers from the independent @maxplanckgesellschaft research group “Binary Merger Observations and Numerical Relativity” have studied how the spins of merging black holes influence the recoil after their merger, and how this in turn influences the remnant spin magnitudes after repeated mergers in dense stellar environments.
The header picture shows some of their results.
ℹ️ https://www.aei.mpg.de/1244528/towards-a-deeper-understanding-of-black-hole-origins?c=785562
📄 https://arxiv.org/abs/2503.21278 (The header picture is Fig. 5 in there)
#HeaderPicture #BlackHoles #BlackHoleKicks #BlackHoleWeek #Astrodon #Astronomy
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🚨 New header picture 🖼️
Researchers from the independent @maxplanckgesellschaft research group “Binary Merger Observations and Numerical Relativity” have studied how the spins of merging black holes influence the recoil after their merger, and how this in turn influences the remnant spin magnitudes after repeated mergers in dense stellar environments.
The header picture shows some of their results.
ℹ️ https://www.aei.mpg.de/1244528/towards-a-deeper-understanding-of-black-hole-origins?c=785562
📄 https://arxiv.org/abs/2503.21278 (The header picture is Fig. 5 in there)
#HeaderPicture #BlackHoles #BlackHoleKicks #BlackHoleWeek #Astrodon #Astronomy
-
🚨 New header picture 🖼️
Researchers from the independent @maxplanckgesellschaft research group “Binary Merger Observations and Numerical Relativity” have studied how the spins of merging black holes influence the recoil after their merger, and how this in turn influences the remnant spin magnitudes after repeated mergers in dense stellar environments.
The header picture shows some of their results.
ℹ️ https://www.aei.mpg.de/1244528/towards-a-deeper-understanding-of-black-hole-origins?c=785562
📄 https://arxiv.org/abs/2503.21278 (The header picture is Fig. 5 in there)
#HeaderPicture #BlackHoles #BlackHoleKicks #BlackHoleWeek #Astrodon #Astronomy
-
🚨 New header picture 🖼️
Researchers from the independent @maxplanckgesellschaft research group “Binary Merger Observations and Numerical Relativity” have studied how the spins of merging black holes influence the recoil after their merger, and how this in turn influences the remnant spin magnitudes after repeated mergers in dense stellar environments.
The header picture shows some of their results.
ℹ️ https://www.aei.mpg.de/1244528/towards-a-deeper-understanding-of-black-hole-origins?c=785562
📄 https://arxiv.org/abs/2503.21278 (The header picture is Fig. 5 in there)
#HeaderPicture #BlackHoles #BlackHoleKicks #BlackHoleWeek #Astrodon #Astronomy
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🚨 New header picture 🖼️
It shows the two supernova remnants Cassiopeia A (left, in X-rays) and Vela Jr. (right, at radio wavelengths). Both harbor a “central compact object”, a neutron star left behind together with the debris cloud after the supernova.
Researchers from the permanent independent @maxplanckgesellschaft research group “Continuous Gravitational Waves” at @mpi_grav in Hanover, Germany, have been searching for gravitational waves from these central compact objects using the volunteer distributed computing project @einsteinathome.
📄 https://arxiv.org/abs/2503.09731
The fact that they did not find any gravitational waves indicates that the neutron stars can only be minimally deformed.
ℹ️ https://www.aei.mpg.de/1188233/digging-deeper-with-einstein-home?c=26149
Images: http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G111.7m02.1 and http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G266.2m01.2
#HeaderPicture #supernova #CasA #VelaJr #astrodon #astronomy #NeutronStar
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🚨 New header picture 🖼️
It shows the two supernova remnants Cassiopeia A (left, in X-rays) and Vela Jr. (right, at radio wavelengths). Both harbor a “central compact object”, a neutron star left behind together with the debris cloud after the supernova.
Researchers from the permanent independent @maxplanckgesellschaft research group “Continuous Gravitational Waves” at @mpi_grav in Hanover, Germany, have been searching for gravitational waves from these central compact objects using the volunteer distributed computing project @einsteinathome.
📄 https://arxiv.org/abs/2503.09731
The fact that they did not find any gravitational waves indicates that the neutron stars can only be minimally deformed.
ℹ️ https://www.aei.mpg.de/1188233/digging-deeper-with-einstein-home?c=26149
Images: http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G111.7m02.1 and http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G266.2m01.2
#HeaderPicture #supernova #CasA #VelaJr #astrodon #astronomy #NeutronStar
-
🚨 New header picture 🖼️
It shows the two supernova remnants Cassiopeia A (left, in X-rays) and Vela Jr. (right, at radio wavelengths). Both harbor a “central compact object”, a neutron star left behind together with the debris cloud after the supernova.
Researchers from the permanent independent @maxplanckgesellschaft research group “Continuous Gravitational Waves” at @mpi_grav in Hanover, Germany, have been searching for gravitational waves from these central compact objects using the volunteer distributed computing project @einsteinathome.
📄 https://arxiv.org/abs/2503.09731
The fact that they did not find any gravitational waves indicates that the neutron stars can only be minimally deformed.
ℹ️ https://www.aei.mpg.de/1188233/digging-deeper-with-einstein-home?c=26149
Images: http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G111.7m02.1 and http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G266.2m01.2
#HeaderPicture #supernova #CasA #VelaJr #astrodon #astronomy #NeutronStar
-
🚨 New header picture 🖼️
It shows the two supernova remnants Cassiopeia A (left, in X-rays) and Vela Jr. (right, at radio wavelengths). Both harbor a “central compact object”, a neutron star left behind together with the debris cloud after the supernova.
Researchers from the permanent independent @maxplanckgesellschaft research group “Continuous Gravitational Waves” at @mpi_grav in Hanover, Germany, have been searching for gravitational waves from these central compact objects using the volunteer distributed computing project @einsteinathome.
📄 https://arxiv.org/abs/2503.09731
The fact that they did not find any gravitational waves indicates that the neutron stars can only be minimally deformed.
ℹ️ https://www.aei.mpg.de/1188233/digging-deeper-with-einstein-home?c=26149
Images: http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G111.7m02.1 and http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G266.2m01.2
#HeaderPicture #supernova #CasA #VelaJr #astrodon #astronomy #NeutronStar
-
🚨 New header picture 🖼️
It shows the two supernova remnants Cassiopeia A (left, in X-rays) and Vela Jr. (right, at radio wavelengths). Both harbor a “central compact object”, a neutron star left behind together with the debris cloud after the supernova.
Researchers from the permanent independent @maxplanckgesellschaft research group “Continuous Gravitational Waves” at @mpi_grav in Hanover, Germany, have been searching for gravitational waves from these central compact objects using the volunteer distributed computing project @einsteinathome.
📄 https://arxiv.org/abs/2503.09731
The fact that they did not find any gravitational waves indicates that the neutron stars can only be minimally deformed.
ℹ️ https://www.aei.mpg.de/1188233/digging-deeper-with-einstein-home?c=26149
Images: http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G111.7m02.1 and http://snrcat.physics.umanitoba.ca/SNRrecord.php?id=G266.2m01.2
#HeaderPicture #supernova #CasA #VelaJr #astrodon #astronomy #NeutronStar
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#Header #Picture
#HeaderPicture
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@fasse
I have to say I really love both your #profilePicture and your #headerPicture a lot!! ❤️