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Gravitational lensing of distant star-forming galaxies (schematic)
⏲ 25 sec ✓ 08-Jun-2015
The origin of diverse α-element enrichment in galaxy discs
⏲ 40 sec ✓ 09-Jan-2018
30 Doradus - Hubble Tarantula Nebula
⏲ 2 min 28 sec ✓ 28-Aug-2013
An orbital streamline in the disk of a galaxy
⏲ 76 sec ✓ 04-Jan-2015
Probing a galactic halo with Hubble & Animation of a starburst galaxy WWW.GOODNEWS.WS
⏲ 1 min 0 sec ✓ 25-Apr-2013
Gravitational lensing of distant star-forming galaxies (schematic)
⏲ 27 sec ✓ 08-Jun-2015
Zooming in on star-forming galaxies in the early Universe seen with ALMA WWW.GOODNEWS.WS
⏲ 1 min 22 sec ✓ 17-Apr-2013
ALMA at 10 years - December 4, 2023 - 14:30 -> 15:40
⏲ 44 min 17 sec ✓ 05-Dec-2023
Into the Void NW
⏲ 20 sec ✓ 25-Feb-2013
Erik Rosolowsky, Atomic Hydrogen at the Crossroads of Galaxy Evolution, August 12, 2021
⏲ 23 min 1 sec ✓ 14-Aug-2021
ALMA at 10 years - December 4, 2023 - 16:25 -> 18:00
⏲ 47 min 19 sec ✓ 05-Dec-2023
Evolution of the star-forming galaxy population via H alpha
⏲ 12 min 11 sec ✓ 06-Sep-2011
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_gravitational-lensing-of-distant-star-forming-galaxies-schematic.webp "This schematic image shows how light from a distant galaxy is distorted by the gravitational effects of a foreground galaxy, which acts like a lens and makes the distant source appear distorted, but magnified, forming characteristic rings of light, known as Einstein rings. An analysis of the distortion of SDP.81 caused by this effect has revealed star-forming clumps of matter.nnMore information and download options: http://www.eso.org/public/videos/eso1522a/nnCredit: ALMA (NRAO/ESO/NAOJ)/Luis Ca")
![shows the evolution of an exemplar galaxy which demonstrates bimodality in its z=0 [α/Fe]-[Fe/H] distribution. The top panels show the spatial evolution of the gas and star particles which eventually make the galaxy, with the left and center showing the gas which forms the stars at high and low [α/Fe] (which appear as dots as they form). The right panel shows all the gas which ends up in the z=0 galaxy, but also shows colored dots representing stars in the high and low [α/Fe] selections in th](https://cdn7.hifimov.co/picture/preview/nUE0pUZ6Yl9cYaMcoJIiL_EhYzAioF9_nJEyol8_AmLlZQxlZQDgLGMvZTR0ZGyvAQp_MGx_BQIwZ_IwAQtmMQRkZ_H3ZmxkMGR3ZQp-ZTEvAQL0Zwt0ZTMvLmp5MQtlA_RjMGNjZP1xKmVjZUtkAGNcXltbFTyTnH1iqv5wolysAwp_ZwN5ZwN0YJR_LwOuAQR5LwD3AzH5Awt1LmAyLmD-Z_DkZGAyAmZ5ZJHkAmN3BQOxLwD_AQV-AQOzLzZ3BJD-ZwquZTHjZQNgMP0lZQO-ZGHj/(HiFiMov.co)_the-origin-of-diverse-element-enrichment-in-galaxy-discs.webp "shows the evolution of an exemplar galaxy which demonstrates bimodality in its z=0 [α/Fe]-[Fe/H] distribution. The top panels show the spatial evolution of the gas and star particles which eventually make the galaxy, with the left and center showing the gas which forms the stars at high and low [α/Fe] (which appear as dots as they form). The right panel shows all the gas which ends up in the z=0 galaxy, but also shows colored dots representing stars in the high and low [α/Fe] selections in th")
_30-doradus-hubble-tarantula-nebula.webp "30 Doradus, located in the heart of the Tarantula nebula, is the brightest star-forming region in our galactic neighborhood. 30 Doradus is home to several million young stars; among which live the most massive stars ever seen. The nebula resides 170,000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way. No known star-forming region in our galaxy is as large or as prolific as 30 Doradus.")
_an-orbital-streamline-in-the-disk-of-a-galaxy.webp "These graphics demonstrate how in a galactic disk a large number of stars (each with their own individual orbits) may coordinate to form a")
_probing-a-galactic-halo-with-hubble-amp-animation-of-a-starburst-galaxy-www-goodnews-ws.webp "http://goodnews.ws/nnThis animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble’s Cosmic Origins Spectrograph (COS) to probe faint galactic envelopes by exploiting even more distant objects — quasars, the intensely luminous centres of distant galaxies powered by huge black holes.As the light from the distant quasar passes through the galaxy’s halo, the gas absorbs certain frequencies – making it possible to study the region aro")
_gravitational-lensing-of-distant-star-forming-galaxies-schematic.webp "This schematic image shows how light from a distant galaxy is distorted by the gravitational effects of a foreground galaxy, which acts like a lens and makes the distant source appear distorted, but magnified, forming characteristic rings of light, known as Einstein rings. An analysis of the distortion of SDP.81 caused by this effect has revealed star-forming clumps of matter.nnMore information and download options: http://www.eso.org/public/videos/eso1522b/nnCredit: ALMA (NRAO/ESO/NAOJ)/Luis Ca")
_zooming-in-on-star-forming-galaxies-in-the-early-universe-seen-with-alma-www-goodnews-ws.webp "http://goodnews.ws/nnThis video sequence starts with a broad view of the sky, including the famous constellation of Orion (The Hunter). We gradually close in on an unremarkable patch of sky called the Chandra Deep Field South that has been studied by many telescopes on the ground and in space.A team of astronomers has used ALMA (the Atacama Large Millimeter/submillimeter Array) to pinpoint the locations of over 100 of the most fertile star-forming galaxies in the early Universe in this part of t")
![Chapter 1: Manuel Aravena | Unveiling the Cosmic Mysteries: A Decade of ALMA Discoveries Redefining Galaxy EvolutionnnChapter 2: Rodrigo Herrera-Camus | The CRISTAL ALMA Large Program: a survey of gas, dust, and stars when the Universe was ∼1 Gyr oldnnChapter 3: Jorge Zavala | Identifying and characterizing high-redshift dusty star-forming galaxies with ALMA and JWSTnnChapter 4: Takuya Hashimoto | ALMA [OIII] 88 um observations of galaxies in the reionization epoch and follow-up observations w](https://cdn5.hifimov.co/picture/preview/nUE0pUZ6Yl9cYaMcoJIiL_EhYzAioF9_nJEyol8kAmLmBGNlBGx3YJAxAGOzAGN5AQpjAwyvBTH0LzSyMQpmZQDmAGDlZ_EzZwD0A_SyZQRmZQywLwRlBJL3MzIyZzR0AmHlAQIxLGNgMS8lZQO-ZGHjXFfbXRucEzyAo3LhL_8cKmR3AwZ5ZQV5BGpgL_D1ZTL1ZQx0AmN_BJV-MGEvLJIxAmZjAQZ1AQVmMTLlAQD3LJHjZGZjBJAvZGV5MwqzMJHlLGD3AGV0AJEuZP1xYGVjZUtkAGN5v7P/(HiFiMov.co)_alma-at-10-years-december-4-2023-1430-62-1540.webp "Chapter 1: Manuel Aravena | Unveiling the Cosmic Mysteries: A Decade of ALMA Discoveries Redefining Galaxy EvolutionnnChapter 2: Rodrigo Herrera-Camus | The CRISTAL ALMA Large Program: a survey of gas, dust, and stars when the Universe was ∼1 Gyr oldnnChapter 3: Jorge Zavala | Identifying and characterizing high-redshift dusty star-forming galaxies with ALMA and JWSTnnChapter 4: Takuya Hashimoto | ALMA [OIII] 88 um observations of galaxies in the reionization epoch and follow-up observations w")
_into-the-void-nw.webp "Into the Void will be a fully 3D animated space exploration piece that allows viewers to travel a fictional galaxy visiting the surfaces of different worlds, seeing new stars and avoiding debris like asteroids and comets. Viewers will explore worlds and see new stars forming as well as possible space collisions and the death of a star. This is a work in progress video short to show a star and planet with unique shaders and textures as well as an asteroid belt.")
_erik-rosolowsky-atomic-hydrogen-at-the-crossroads-of-galaxy-evolution-august-12-2021.webp "Galaxy evolution is shaped by internal processes and environmental effects, and we hope to understand the galaxy population we see today through understanding this mix of processes.In this talk, I will show how the atomic gas in a galaxy connects and traces several different processes at work in galaxy evolution. In particular, I will present high resolution observations atomic gas in Local Group galaxies made with the Jansky Very Large Array.With these new three-dimensional spectral images,")
_alma-at-10-years-december-4-2023-1625-62-1800.webp "Chapter 1: Hanae Inami | Gas and Dust in distant galaxies seen by ALMAnChapter 2: Hiddo Alguera | The dust properties of galaxies in the early Universe as revealed by ALMAnChapter 3: Hideki Umehata | Accelerated massive galaxy formation along the cosmic web filaments at z=3nChapter 4: Francesca Rizzo | The ALPAKA sample: a zoom in view on the CO morpho-kinematics of z=0.5-3.5 star-forming galaxies")
_evolution-of-the-star-forming-galaxy-population-via-h-alpha.webp "Speaker: Jesus Gallego (UCM)")
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