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#Astrodon

37 posts30 participants4 posts today

02/04/2025 - Evening walk up Tap o' Noth in Aberdeenshire. We took the scope and spent 4hrs on top, just sitting, having a brew and chatting to the stars. It was chilly but we hid behind the ramparts so it was OK (there's a Pictish hillfort on top). Aurora, stars, galaxies and nebula on a dark night, it was all pretty magic.

✨ New selected research highlight ✨

Towards a deeper understanding of black hole origins

Research team studies the impact of remnant kicks on spin distributions of black holes from hierarchical mergers

A new study revisits modelling of the spin distributions from hierarchical binary black hole mergers in dense stellar environments, such as globular clusters. It finds clear deviations from the unique spin distribution described in previous studies, and shows a way to identify black holes from repeated mergers, which could help shed light on black hole formation through precise spin measurements in future observing runs.

Read more ➡️ aei.mpg.de/1244528/towards-a-d

📄 arxiv.org/abs/2503.21278

I took this back on the 10th of March.

It is our old friend the Eta Carinae Nebula.

This time with a SII/OIII filter (thanks for the suggestion, @malcircuit !) and 120x90s@80 for the exposures. Then I ran it through the Dwarflab star removal tool, and post-processed the result in Snapseed.

I was not going to post it, but it came up as a background on my office screen today (long story), and I had not realised just how much detail it had.

🚨 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.

📄 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 aei.mpg.de/1188233/digging-dee

Images: snrcat.physics.umanitoba.ca/SN and snrcat.physics.umanitoba.ca/SN

🚨 Neues Header-Bild 🖼️

Es zeigt die beiden Supernova-Überreste Cassiopeia A (links, im Röntgenbereich) und Vela Jr. (recht, im Radiobereich). Beide beherbegen ein „zentrales kompaktes Objekt“, einen Neutronenstern, der mit der Explosionswolke nach der Supernova zurückblieb.

Forschende der dauerhaften unabhängigen @maxplanckgesellschaft Forschungsgruppe „Kontinuierliche Gravitationswellen“ am @mpi_grav in Hannover haben mit dem verteilten Rechenprojekt @einsteinathome nach Gravitationswellen von diesen zentralen kompakten Objekten gesucht.

📄 arxiv.org/abs/2503.09731

Dass sie keine Gravitationswellen gefunden haben, verrät, dass die Neutronensterne nur minimal verformt sein können.

ℹ️ aei.mpg.de/1188233/digging-dee

Bilder: snrcat.physics.umanitoba.ca/SN bzw. snrcat.physics.umanitoba.ca/SN