Paola Domínguez(@PaolaDom1) 's Twitter Profileg
Paola Domínguez

@PaolaDom1

Astrophysicist at @CenterForAstro | @Harvard 🌌
Hecha en #UNAM. PhD at the University of Hamburg |🇲🇽🇩🇪| 🇰🇷 | 🇮🇹

ID:1004105220505456641

linkhttp://paoladominguez-fernandez.me calendar_today05-06-2018 20:58:34

455 Tweets

449 Followers

672 Following

CERN(@CERN) 's Twitter Profile Photo

It is with great sadness that we learned of the passing of Peter Higgs.

An iconic figure in modern science, Higgs postulated the existence of the eponymous Higgs boson in 1964. Its discovery at CERN in 2012 was the crowning achievement of the Standard Model of particle physics –…

It is with great sadness that we learned of the passing of Peter Higgs. An iconic figure in modern science, Higgs postulated the existence of the eponymous Higgs boson in 1964. Its discovery at CERN in 2012 was the crowning achievement of the Standard Model of particle physics –…
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Dr. James Beattie(@astro_magnetism) 's Twitter Profile Photo

Plasmoid instabilities in current sheets are ubiquitous in high Rm turbulence, regardless of whether turbulent reconnection is realized or not. That’s what the data says. Pictured below is the current sheet structure in MHD turbulence with Rm ~ 3 x 10^6.

Plasmoid instabilities in current sheets are ubiquitous in high Rm turbulence, regardless of whether turbulent reconnection is realized or not. That’s what the data says. Pictured below is the current sheet structure in MHD turbulence with Rm ~ 3 x 10^6.
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Monika M.(@mmosc_m) 's Twitter Profile Photo

Proudly presenting brand new image of Sgr A* supermassive black hole. This time in polarized light, unveiling magnetic fields around the event horizon of Sgr A*. Only Event Horizon 'Scope can give us access to such detail view of conditions near black holes. eventhorizontelescope.org/blog/astronome…

Proudly presenting brand new image of Sgr A* supermassive black hole. This time in polarized light, unveiling magnetic fields around the event horizon of Sgr A*. Only @ehtelescope can give us access to such detail view of conditions near black holes. eventhorizontelescope.org/blog/astronome…
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Andrea Botteon(@and_botteon) 's Twitter Profile Photo

Our (Vazza+myself) review is on arxiv
We provide a concise overview of the observational+theoretical knowledge of the seeding of cosmic ray electrons by cluster radio galaxies. This field is rapidly evolving: we believed that is was time to make the point
arxiv.org/abs/2403.16068

Our (Vazza+myself) review is on arxiv We provide a concise overview of the observational+theoretical knowledge of the seeding of cosmic ray electrons by cluster radio galaxies. This field is rapidly evolving: we believed that is was time to make the point arxiv.org/abs/2403.16068
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Andrea Botteon(@and_botteon) 's Twitter Profile Photo

Radio/X-ray study of cool-core clusters, by Biava+
The connection between sloshing, cold fronts, mini halos and diffuse radio emission on broader scale is investigated with Low Frequency Array and Chandra Observatory in 12 clusters. Sloshing is key for diffuse radio emission!
arxiv.org/abs/2403.09802

Radio/X-ray study of cool-core clusters, by Biava+ The connection between sloshing, cold fronts, mini halos and diffuse radio emission on broader scale is investigated with @LOFAR and @chandraxray in 12 clusters. Sloshing is key for diffuse radio emission! arxiv.org/abs/2403.09802
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Chiara Stuardi(@CStuardi) 's Twitter Profile Photo

Our paper about magnetic fields in galaxy clusters was chosen for the Nature Communications Editors' Highlights nature.com/collections/bb…

Thank you Nilda Oklay Vincent for chosing our results!!

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Andrea Botteon(@and_botteon) 's Twitter Profile Photo

AGN-feeback in high-z clusters, by Timmerman+ (including myself)
By combining high-resolution observations with Low Frequency Array long baselines + Chandra Observatory it is possible to push measuraments of Pcav at z>0.6. Here we report detections of radio lobes up to z=0.9!
arxiv.org/abs/2403.03242

AGN-feeback in high-z clusters, by Timmerman+ (including myself) By combining high-resolution observations with @LOFAR long baselines + @chandraxray it is possible to push measuraments of Pcav at z>0.6. Here we report detections of radio lobes up to z=0.9! arxiv.org/abs/2403.03242
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Andrea Botteon(@and_botteon) 's Twitter Profile Photo

MeerKAT-meets-LOFAR..for A2142, by Chris Riseley+ (w/ Annalisa Mariachiara Rossetti FraLoi Dr Tessa Vernstrom myself++)
Radio+X-ray data are used to study the connection between thermal and non-thermal components, confirming that this is quite a complex system
arxiv.org/abs/2403.00414

MeerKAT-meets-LOFAR..for A2142, by @cjriseley+ (w/ @AnnalisBonafede @mcrossetti_twit @FraLoi1 @tvern23 myself++) Radio+X-ray data are used to study the connection between thermal and non-thermal components, confirming that this is quite a complex system arxiv.org/abs/2403.00414
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Fabio Gastaldello(@fabiogasta) 's Twitter Profile Photo

CHEX-MATE minisplash of papers today ! arxiv.org/abs/2402.18654 Balboni lead a pilot project with 5 radio halo clusters observed with Low Frequency Array and ESA XMM-Newton to study non-thermal properties in a spatially resolved fashion. 1

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Astro Plot of the Week(@PlotAstro) 's Twitter Profile Photo

We have the newest 'Astro Plot of the Week' - congratulations!

And keep them coming: astro plots >> other plots 😀

We have the newest 'Astro Plot of the Week' - congratulations! And keep them coming: astro plots >> other plots 😀
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