https://www.youtube.com/watch?v=fDUOEdcjqSo
What are massive stars and supernovae, and why are they so rare? And why have they had such a huge effect on the evolution of the universe?Watch the Q&A her

https://www.rigb.org/explore-science/explore/video/massive-stars-and-supernovae-thomas-haworth
Massive stars, around 40 times larger than the sun, emit vast amounts of energy which heats and blows away the star-forming gas. In this talk, Thomas Haworth shares the latest understandings of how the energy from massive stars is impacting the clusters and galaxies around them. From the destruction of planet-forming discs surrounding young

https://www.facebook.com/royalinstitution/videos/what-are-massive-stars-thomas-haworth/833828741456859/
The sun is really big, but there are massive stars 40 times bigger, affecting space all around them. Thomas Haworth tells us more about how they are formed. See less

https://sciencereader.com/video/massive-stars-and-supernovae-with-thomas-haworth/
In this thought-provoking Q&A session, astrophysicist Thomas Haworth explores the impact of massive stars and supernovae on the evolution of the universe, revealing their rarity, immense power, and significant contributions to the diversity of planets, taking viewers on an awe-inspiring journey through stellar formation, energy surges, and the destruction caused by these celestial powerhouses.

https://www.classcentral.com/course/youtube-massive-stars-and-supernovae-with-thomas-haworth-202991
Explore the formation and impact of massive stars and supernovae on the universe in this 1-2 hour material from The Royal Institution, led by Thomas Haworth. BloomTech's Downfall: A Long Time Coming

https://www.rigb.org/whats-on/supernova-science-destruction-stars
Massive stars, around 40 times larger than the sun, emit vast amounts of energy which heats and blows away the star-forming gas. In this talk, Thomas Haworth shares the latest understandings of how the energy from massive stars is impacting the clusters and galaxies around them. From the destruction of planet-forming discs surrounding young

https://www.reddit.com/r/space/comments/14seibc/massive_stars_and_supernovae_with_thomas_haworth/
What are massive stars and supernovae, and why are they so rare? And why have they had such a huge effect on the evolution of the universe? Advertisement Coins. 0 coins. Premium Powerups Explore Gaming. Valheim Genshin Impact ... Massive stars and supernovae - with Thomas Haworth.

https://www.seresearch.qmul.ac.uk/cfp/people/thaworth
Warm millimetre dust in protoplanetary discs near massive stars. Monthly Notices of the Royal Astronomical Society, Oxford University Press ... From Supernovae to Planet Formation. The Astronomical Journal, American Astronomical Society vol. 160 (6), ... Thomas James Haworth £1,676,608 EPSRC - EU Scheme (01-01-2024

https://www.linkedin.com/posts/qmul-science-and-engineering_massive-stars-and-supernovae-with-thomas-activity-7097143500508393472-D0YC
Massive stars are the most powerful ones in the universe, but they also have the shortest lifespans. In this talk by Dr Thomas Haworth at the The Royal InstitutionThomas Haworth at the The Royal

https://www.newscientist.com/article/mg25734331-200-dont-miss-a-supernova-science-talk-by-astrophysicist-thomas-haworth/
Visit. Supernova Science really matters, as the destructive effects of exploding stars wreak havoc across the universe. Astrophysicist Thomas Haworth explains at the Royal Institution, London, at

https://clipzag.com/watch?v=fDUOEdcjqSo
However, alongside the creation there is destruction. Massive stars, around 40 times larger than the sun, emit vast amounts of energy which heats and blows away the star-forming gas. In this talk, Thomas Haworth shares the latest understandings of how the energy from massive stars is impacting the clusters and galaxies around them.

https://www.linkedin.com/posts/hunt-eliza_massive-stars-and-supernovae-with-thomas-activity-7097253928882376704-1H5C
Massive stars are the most powerful ones in the universe, but they also have the shortest lifespans. In this talk by Dr Thomas Haworth at the The Royal Institution, we learn about their secret

http://cosmo.uchicago.edu/comptonlectures/humensky/68thSeriesLecture4.pdf
Fusion in Massive Stars. Massive stars (tt8 M8 MŸ ) go through many fusion stages beyond ) go through many fusion stages beyond 44He:He: For a 25 M Ÿ. starstar. Compare: water density is 1000 kg/m33 = 1 * 10= 1 * 103 kg/mkg/m3. Stages require increasingly higher temperatures and densities.

https://thaworth.wixsite.com/astro/publications
Olja Panić, Thomas J. Haworth, et al., 2021, MNRAS, 501, 4317 22. An ALMA survey of Lambda Orionis discs: from supernovae to planet formation. Megan Ansdell, Thomas J. Haworth, et al., 2020, MNRAS, 160, 248 23. Testing viscous disc theory using the balance between stellar accretion and external photoevaporation of protoplanetary discs

https://orcid.org/0000-0002-9593-7618
Diffuse thermal X-ray emission from bow shocks of massive stars. Zenodo 2022-11-08 | Other ... From Supernovae to Planet Formation. The Astronomical Journal 2020-12-01 ... 10.3847/1538-3881/abb9af Contributors: Megan Ansdell; Thomas J. Haworth; Jonathan P. Williams; Stefano Facchini; Andrew Winter;

https://www.cfa.harvard.edu/news/superluminous-supernova
A Superluminous Supernova. An artist's depiction of a magnetar, the dense, highly magnetized residue of some types of supernova explosions. Observations of a superluminous supernova suggest that its remnant is a magnetar. Supernovae are the explosive deaths of massive stars. Among the most momentous events in the cosmos, they disburse into

https://en.wikipedia.org/wiki/Near-Earth_supernova
The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.It is located about 6,500 light-years from the Earth. A near-Earth supernova is an explosion resulting from the death of a star that occurs close enough to the Earth (roughly less than 10 to 300 parsecs [30 to 1000 light-years] away) to have noticeable effects on Earth's biosphere.

https://link.springer.com/referenceworkentry/10.1007/978-3-319-20794-0_119-1
3.1 Core H Burning. Core H burning is the first stable and long-lasting nuclear burning stage. In massive stars with initial metallicity \(\mathrm{Z} \gtrsim 10^{-7}\), it occurs at temperatures of the order of ∼ 4 to ∼ 6 ⋅ 10 7 K, and therefore it is powered by the CNO cycle.The high sensitivity of the CNO cycle on the temperature implies a high nuclear energy flux and hence the

https://arxiv.org/abs/1709.03207
Almost since the beginning, massive stars and their resultant supernovae have played a crucial role in the Universe. These objects produce tremendous amounts of energy and new, heavy elements that enrich galaxies, encourage new stars to form and sculpt the shapes of galaxies we see today. The end of millions of years of massive star evolution and the beginning of hundreds or thousands of years

https://pubmed.ncbi.nlm.nih.gov/28923995/
Abstract. Almost since the beginning, massive stars and their resultant supernovae have played a crucial role in the Universe. These objects produce tremendous amounts of energy and new, heavy elements that enrich galaxies, encourage new stars to form and sculpt the shapes of galaxies that we see today. The end of millions of years of massive

https://www.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2018.00025/pdf?isPublishedV2=false
The death of massive stars, manifested as gamma-ray bursts and core-collapse supernovae, critically influence how the universe formed and evolves. Despite their fundamental importance, our understanding of these enigmatic objects is severely limited. We have performed a concept study of an Astrophysical Transient Observatory

https://spacenews.com/image-the-cool-clouds-of-carina/
A prime example of these violent stars is Eta Carinae, the bright yellowish star just to the upper left of the centre of the image. It has over 100 times the mass of our Sun, and is among the most

https://www.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2018.00025/full
The death of massive stars, manifested as gamma-ray bursts and core-collapse supernovae, critically influence how the universe formed and evolves. ... J. Bayless 3 Volker Bromm 4 Peter J. Brown 5 Michael W. Davis 3 Anastasia Fialkov 6 Brian Fleming 7 Kevin France 7 Chris L. Fryer 8 Thomas K. Greathouse 3 Jed J. Hancock 9 D. Andrew Howell 10,11