Gaia View on a Heartless Starcluster in Cross Section =New physics supported by the "New Penrose-Q-FFF Black Holes " creating AND even repelling all Fermions.

Omega Centauri, the largest globular cluster that can be seen from Earth and a great example of a ‘typical’ Globular Cluster.

Mystery of the empty center is Solved, by the new Penrose -Q-FFF Black Hole, postulating that each black hole consumes Photons and the vacuum virtual space frame, but REPEL Massive particles like stars leaving a Hole inside all Starclusters. see also: 

https://vixra.org/author/leo_vuyk 

This image shows a star cluster, which appears as a collection of bright stars against a dark background. The roughly circular cluster appears like a doughnut with an empty centre. see: https://www.esa.int/ESA_Multimedia/Images/2023/10/Gaia_view_of_Omega_Centauri_Data_Release_3

Gaia's discovery of the century: The Heartless Globular Cluster, pointing to  the New Physics of the Dark Matter Black Hole Big Bang based on the new Penrose-Q-FFF Black Hole Model, leading to Dual String Gravity and a Theory of everything.

Look at the empty center (left) of the Ball Cluster: "On the right, this emptiness has been filled, with so many stars present that the core appears to be almost solidly bright rather than comprising individual stars. "

My Conclusion: 

The central super massive black hole is lensing the surrounding stars in all directions showing no individual stars any more in the center . (see; "almost solidly bight rather than comprising individual stars")

Below, the Hole inside the Blobular Starcluster. showing much less stars in the empty center by the rearly Big Bang Black Hole..(supported by the Q-FFF model)

However, the center is overcrowded by star light that is deflected by the central black hole!! SO we see: light from around all stars, which is the concentation result of the Black Hole LENSING BY THE CENTRAL MASSIVE BLACK HOLE. THIS HOLE IS CALLED A GABH (one of the two Galaxy Anchor Black Holes of a former merger galaxy)

Below: The outside of the Omega Centauri Globular Cluster.

Today, ESA's Gaia mission releases a goldmine of knowledge about our galaxy and beyond in its 'focused product release'. Among other findings, the star surveyor reveals more than half a million faint stars in a massive cluster – stars the telescope had not seen before.

Gaia’s third data release (DR3) contained data on over 1.8 billion stars, building a pretty complete view of the Milky Way and beyond. However, there remained gaps in our mapping. Gaia had not yet fully surveyed areas of sky that were especially densely packed with stars, leaving these comparatively unexplored – and overlooking stars shining less brightly than their many neighbours.

To patch the gaps in our maps, Gaia selected Omega Centauri, the largest globular cluster that can be seen from Earth and a great example of a ‘typical’ cluster. Rather than just focusing on individual stars as it typically would, Gaia enabled a special mode to truly map a wider patch of sky surrounding the cluster’s core every time the cluster came into view.

The team revealed 526 587 new Gaia stars from this cluster alone, detecting stars that lie too close together to be measured in the telescope’s regular pipeline and those in the cluster core that are up to 15 times fainter than previously seen. The new data reveal 10 times more stars in Omega Centauri; this new knowledge will enable researchers to study the cluster’s structure, how the constituent stars are distributed, how they’re moving, and more, creating a complete large-scale map of Omega Centauri.

Gaia is exploring nine crowded regions in this way, with the full results expected in Gaia Data Release 4. 

The image of Omega Centauri in this infographic, in the inset circle, shows the cluster as observed by Gaia. Stars of all brightnesses are visible within.

Below: Starcluster distribution (Theory) all around Galaxies like Andromeda and the Milky way are the result of early DUAL GABHs (Galaxy Anchor Black Holes) being former Herbig Haro Bowshock black holes with a galaxy in the middle later merged into the Milky Way and Andromeda.

Where these GABHs come from? 

According to Q-FFF Theory, The Big Bang was the explosion of the central Singularity dark matter black hole into smaller chuncks of black holes.

The Q-FFF Theory postulate, that each black hole do create and repel Fermion Plasma, at the new physics "Penrose-Q-FFF Horizon" and do not consume mass ( Fermions).

Globular Starclusters seem to be great subjects to show this new physics effect by the nearly empty center of the Starcluster.

Tadpole Black Hole creating stars and searching for a second Black Hole for merging or creating a Herbig Haro dual Black Hole.

The principle of the Tadpole Black Hole cruising through space forming mergers or dual Herbig Haro systems forming stars in the middle .

From the press:  SCIENCE & EXPLORATION

10 times more stars: Comparing two Gaia views of Omega Centauri (slider)

10/10/2023409 VIEWS12 LIKES483140 ID

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ESA's star-surveying Gaia mission has released a treasure trove of new data as part of its ‘focused product release’. As part of this data release Gaia explored Omega Centauri, the largest globular cluster that can be seen from Earth and a great example of a ‘typical’ cluster.  

The team has revealed 526 587 stars that Gaia had not seen before, detecting stars that lie too close together to be measured in the telescope’s regular pipeline and those in the cluster core that are up to 15 times fainter than previously seen. The new data reveal 10 times more stars in Omega Centauri; this new knowledge will enable researchers to study the cluster’s structure, how the constituent stars are distributed, how they’re moving, and more. 

The image on the left is from Gaia’s Data Release 3 in 2022. The image on the right is from today’s data release, and shows just how many new sources have been imaged in the cluster’s centre. Only faint stars within Omega Centauri are plotted in both images.  

Read more 

Alt-text: This slider image compares two views of a star cluster, which appears as a collection of bright stars against a dark background. On the left, the roughly circular cluster appears like a doughnut with an empty centre. On the right, this emptiness has been filled, with so many stars present that the core appears to be almost solidly bright rather than comprising individual stars. 

Acknowledgments: Michele Trabucchi, Nami Mowlavi and Thomas Lebzelter