Nature Astronomy
@natastron.nature.com
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A Nature journal dedicated to presenting the very best research across the disciplines of astronomy, astrophysics, cosmology and planetary science.📡 www.nature.com/natastron
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natastron.nature.com
Our June(teenth) issue is now here to read: https://bit.ly/3ZI5VOV
The cover image depicts a ticking time bomb... a supernova progenitor on our doorstep! But don't worry, we still have a good 20 billion years until it goes bang.
Two luminescent blue-ish white dwarf stars interact through a transfer of a plasma stream. One star is surrounded by reddish ejecta; the other appears distorted.
Reposted by Nature Astronomy
astromagnetism.bsky.social
@natastron.nature.com’s cover looks amazing this month! Read more about our study on interstellar turbulence here: www.nature.com/articles/s41...
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mpi-astro.bsky.social
1/ 🔭 Massive stars often come in pairs – even in the early #Universe
A new study led by H. Sana (KU Leuven), with contributions from MPIA‘s Jaime Villaseñor @jvillasr.bsky.social, reveals that most massive stars in the Small Magellanic Cloud #SMC have a close partner star.
#Astronomy #MassiveStars
Massive star in metal-poor environment often have close partner
Massive stars in metal-poor galaxies often have close partners, just like the massive stars in our metal-rich Milky Way. This is discovered by an international team of seventy astronomers, co-led by P...
fys.kuleuven.be
Reposted by Nature Astronomy
eso.org
ESO @eso.org · Jul 2
💥💥 Double detonation! 

For the first time, astronomers have obtained visual evidence that a star met its end by detonating twice.

The fingerprint that points to this mechanism is represented by two separate shells of calcium.  

Read more: https://www.eso.org/public/news/eso2511/

🔭 🧪 ☄️ 1/
A view of the remnants of a supernova explosion, featuring two concentric rings of ejected material. The outer ring glows in warm orange tones, while the inner ring is blue. The object is set against a dark backdrop sprinkled with distant stars.
natastron.nature.com
This month we highlight a score of Black astronomers trying to pursue their ambitions without fear, and Black In Astro, an organization supporting predominantly early-career Black people working in the space sciences. Editorial: www.nature.com/articles/s41... #BlackSpaceWeek #EquityInSTEM 🔭
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natastron.nature.com
Our June(teenth) issue is now here to read: https://bit.ly/3ZI5VOV
The cover image depicts a ticking time bomb... a supernova progenitor on our doorstep! But don't worry, we still have a good 20 billion years until it goes bang.
Two luminescent blue-ish white dwarf stars interact through a transfer of a plasma stream. One star is surrounded by reddish ejecta; the other appears distorted.
natastron.nature.com
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natastron.nature.com
Apologies about the formatting of that post 🤔
Reposted by Nature Astronomy
blackinastro.bsky.social
Schedule for #BlackSpaceWeek 2025! Links to register coming soon🤭 Which event/panels pique your interest? 👀
Image promoting #BlackSpaceWeek 2025, scheduled for June 15–21. Each day has a theme and event:
	•	June 15, Sunday: #IntroducingTheUniverse – Virtual mixer and reading with StriveHigher
	•	June 16, Monday: #PicturingTheUniverse – Black in Planetarium Panel
	•	June 17, Tuesday: #AccessingTheUniverse – Black in Space Policy Panel
	•	June 18, Wednesday: #SharingTheUniverse – Black in Journalism Panel
	•	June 19, Thursday: #ShowcasingTheUniverse – Social Media Scavenger Hunt
	•	June 20, Friday: #ReadingTheUniverse – Black in Storytelling Panel
	•	June 21, Saturday: #CraftingTheUniverse – Virtual Craft Night
Background features a starry sky. Logo includes a purple raised fist with “BIA.” Graphic by @CheyennePolius, website: www.blackinastro.com.
natastron.nature.com
Using LAMOST data, Yu et al. find that binary stars with orbital periods < 1 day show enhanced magnetic activity compared to single stars, along with supersaturation. These findings constrain poorly understood dynamo processes in contact binaries.
Enhanced magnetic activity in rapidly rotating binary stars - Nature Astronomy
Binary stars with orbital periods of less than a day show magnetic activity beyond the saturation limit of single stars. This enhanced activity is probably driven by a large-scale α–ω dynamo during common-envelope evolution.
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