Tag Archive for 'Star formation'

An artist’s impression of a runaway supermassive black hole that was ejected from its host galaxy as a result of a tussle between it and two other black holes. Image credit: NASA / ESA / Leah Hustak, STScI.

Hubble Spots Runaway Supermassive Black Hole

Apr 11, 2023 by Enrico de Lazaro

The newly-discovered supermassive black hole resides in a compact star-forming galaxy around 7.7 billion years away and has a mass of 20 million solar...

This Hubble image shows the jellyfish galaxy JW100 (seen edge-on in the lower right). Image credit: NASA / ESA / Hubble / M. Gullieuszik / GASP Team.

Hubble Focuses on Jellyfish Galaxy JW100

Mar 20, 2023 by Enrico de Lazaro

Streams of star-forming gas dripping from the disk of a spiral galaxy called JW100 are formed by a process called ram pressure stripping, and their resemblance...

V883 Orionis is a unique protostar whose temperature is just hot enough that the water in its circumstellar disk has turned to gas, making it possible for radio astronomers to trace the water’s origins. Image credit: ESO / L. Calçada.

Deuterium-Enriched Water Ties Protoplanetary Disks to Comets and Protostars

Mar 9, 2023 by News Staff

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have detected gaseous water in the planet-forming disk around V883 Orionis, a...

Multiwavelength detection of the X3 system with NIRC2 instrument at the W.M. Keck Observatory in 2019. Image credit: Peißker et al., doi: 10.3847/1538-4357/aca977.

Massive Protostar Spotted near Milky Way’s Supermassive Black Hole

Mar 1, 2023 by Natali Anderson

X3a is approximately 10 times larger than the Sun, 15 times as massive, and is only several tens of thousands of years old. Multiwavelength detection of...

This Hubble image shows the spiral galaxy NGC 5033. The image is a composite of separate exposures acquired by Hubble’s Advanced Camera for Surveys (ACS). It is based on data obtained through two filters. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / Judy Schmidt, www.geckzilla.com.

ALMA Detects Supermassive Black Hole in Early Star-Forming Galaxy

Feb 28, 2023 by News Staff

Astronomers using the Atacama Large Millimeter Array (ALMA) have detected a rapidly growing supermassive black hole in COS-87259, a galaxy that forms stars...

This Hubble image shows JO201 (also known as Ka 364, LEDA 2456 and LEDA 93189), a jellyfish galaxy located in the constellation of Cetus. Image credit: NASA / ESA / Hubble / M. Gullieuszik.

Hubble Finds Star-Forming Clumps in Six Jellyfish Galaxies

Feb 27, 2023 by Natali Anderson

Astronomers using the NASA/ESA Hubble Space Telescope have observed clumps of star formation in the tails and disks of six ram-pressure stripped (jellyfish)...

This Webb image shows NGC 7496, a barred spiral galaxy some 24 million light-years away in the constellation of Grus. Image credit: NASA / ESA / CSA / Webb / Judy Schmidt.

Webb Focuses on Polycyclic Aromatic Hydrocarbons in Nearby Galaxies

Feb 16, 2023 by News Staff

Webb observations of polycyclic aromatic hydrocarbon emission provide some of the deepest and highest resolution views of the cold interstellar medium...

The radio image of SDSS J0826+5630. Image credit: Chakraborty & Roy, doi: 10.1093/mnras/stac3696.

Astronomers Detect Radio Signal from Strongly Gravitationally Lensed Galaxy

Jan 18, 2023 by News Staff

Using archival data from the Giant Metrewave Radio Telescope, astronomers have captured a radio signal at a specific wavelength known as the 21 cm line...

This image, taken by the Near-Infrared Camera (NIRCam) onboard the NASA/ESA/CSA James Webb Space Telescope, shows the star cluster NGC 346. Webb reveals the presence of many more building blocks than previously expected, not only for stars, but also planets, in the form of clouds packed with dust and hydrogen. The plumes and arcs of gas in this image contains two types of hydrogen. The pink gas represents energized hydrogen, which is typically as hot as around 10,000 degrees Celsius (approximately 18,000 degrees Fahrenheit) or more, while the more orange gas represents dense, molecular hydrogen, which is much colder at around minus 200 degrees Celsius or less (approximately minus 300 degrees Fahrenheit), and associated dust. The colder gas provides an excellent environment for stars to form, and, as they do, they change the environment around them. The effect of this is seen in the various ridges throughout, which are created as the light of these young stars breaks down the dense clouds. The many pillars of glowing gas show the effects of this stellar erosion throughout the region. In this image blue was assigned to the wavelength of 2.0 microns (F200W), green was assigned to 2.77 microns (F277W), orange was assigned to 3.35 microns (F335M), and red was assigned to 4.44 microns (F444W). Image credit: NASA / ESA / CSA / O. Jones, UK ATC / G. De Marchi, ESTEC / M. Meixner, USRA / A. Pagan, STScI / N. Habel, USRA / L. Lenkic, USRA / L. Chu, NASA’s Ames Research Center.

Webb Probes Most Massive Star-Forming Region of Small Magellanic Cloud

Jan 13, 2023 by Enrico de Lazaro

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have revealed many new pockets of star formation in NCG 346, an open star cluster in the...

This Hubble image shows a part of the Carina Nebula, which is located 7,500 light-years away in the southern constellation of Carina. Image credit: NASA / ESA / A. Kraus, University of Texas at Austin / Gladys Kober, NASA & Catholic University of America.

Hubble Space Telescope Zooms in on Carina Nebula

Dec 28, 2022 by Enrico de Lazaro

NASA has released a sparkling photo taken by the NASA/ESA Hubble Space Telescope of a small section of the Carina Nebula. This Hubble image shows a part...

$This Webb image shows NGC 7469, a barred spiral galaxy some 206 million light-years away in the constellation of Pegasus. The galaxy has blue-purple hues with orange-red regions filled with stars. NGC 7469’s companion galaxy, IC 5283, is partly visible in the lower left portion of this image. Also visible is large diffraction spike, which appears as a star pattern over the central region of the galaxy. Lots of stars and galaxies fill the background scene. Image credit: NASA / ESA / CSA / Webb / L. Armus / A.S. Evans.$

Webb Studies Star Formation in NGC 7469

Dec 21, 2022 by Enrico de Lazaro

NGC 7469 is a very luminous, face-on barred spiral galaxy approximately 90,000 light-years in diameter. This Webb image shows NGC 7469, a barred spiral...

This Webb image shows the Cosmic Cliffs, a region at the edge of a gigantic, gaseous cavity within the stellar nursery NGC 3324. The image is divided horizontally by an undulating line between a orange-burgundy cloudscape forming a nebula along the bottom portion and a comparatively blue upper portion. Image credit: NASA / ESA / CSA / STScI / J. DePasquale, STScI.

Webb Reveals Protostars and Energetic Jets in ‘Cosmic Cliffs’

Dec 20, 2022 by Enrico de Lazaro

Using the images from the NASA/ESA/CSA James Webb Space Telescope, astronomers have discovered 24 previously shrouded outflows from newborn stars in the...

This Hubble image shows a free-floating evaporating gaseous globule (small tadpole-shaped dark region in the upper center-left) within the emission nebula Westerhout 5. Image credit: NASA / ESA / Hubble / R. Sahai.

Hubble Spots Free-Floating Globule in Westerhout 5

Dec 19, 2022 by Enrico de Lazaro

The Hubble team has released an incredibly beautiful image taken by the NASA/ESA Hubble Space Telescope of a small portion of the large emission nebula...

This Webb image shows the center of Messier 74. Image credit: NASA / ESA / CSA / Webb / Hoyer et al., arXiv: 2211.13997.

Webb Focuses on Nuclear Star Cluster of Messier 74

Nov 30, 2022 by Natali Anderson

Using new images from the NASA/ESA/CSA James Webb Space Telescope as well as archival data from the NASA/ESA Hubble Space Telescope, astronomers have studied...

TMC-1. Image credit: ESA / Herschel / NASA / JPL-Caltech / R. Hurt, JPL-Caltech.

Astronomers Detect Two New Organic Molecules in Interstellar Medium

Nov 7, 2022 by Natali Anderson

Astronomers using the 40-m radio telescope at Yebes Observatory have detected two new complex molecules, butadiynethionyl (HCCCCS) and ethynylbutatrienyliden...

IC 1623 is approaching the final stage of its merger, when a violent central inflow of gas will trigger intense starburst activity that could boost the infrared luminosity above the ultraluminous threshold. Image credit: NASA / ESA / CSA / Webb / L. Armus / A. Evans / R. Colombari.

Webb Observes Interacting Galaxy System IC 1623

Oct 26, 2022 by Natali Anderson

NASA has released a stunning image snapped by the NASA/ESA/CSA James Webb Space Telescope of IC 1623, an ongoing cosmic collision between two irregular...

Bohn et al. identified a new set of previously undetected star-forming regions that are heavily obscured by dust in a starburst ring in the barred spiral galaxy NGC 7469. The area of this image from Webb’s Near-Infrared Camera (NIRCam) is shown by a box in the image of NGC 7469 below. Image credit: Bohn et al., arXiv: 2209.04466

Webb Observes Powerful Starburst Ring in NGC 7469

Sep 14, 2022 by Natali Anderson

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have discovered 36 new star-forming regions in a circumnuclear starburst ring in the barred...

This image, taken by the Dark Energy Camera on the Víctor M. Blanco 4-m telescope at Cerro Tololo Inter-American Observatory, shows the Lobster Nebula. Image credit: CTIO / NOIRLab / DOE / NSF / AURA / T.A. Rector, University of Alaska Anchorage & NSF’s NOIRLab / J. Miller, Gemini Observatory & NSF’s NOIRLab / M. Zamani & D. de Martin, NSF’s NOIRLab.

Dark Energy Camera Celebrates Its 10th Birthday with Stunning Photo of Lobster Nebula

Sep 13, 2022 by Enrico de Lazaro

The Dark Energy Camera (DECam), a 570-megapixel U.S. Department of Energy-fabricated camera mounted on the Víctor M. Blanco 4-m telescope at NOIRLab’s...

The inner region of the Orion Nebula as seen by the NIRCam instrument on board the NASA/ESA/CSA James Webb Space Telescope. This is a composite image from several filters that represents emission from ionized gas, hydrocarbons, molecular gas, dust and scattered starlight. Most prominent is the Orion Bar, a wall of dense gas and dust that runs from the top left to the bottom right in this image, and that contains the bright star θ2 Orionis A. The scene is illuminated by a group of hot, young massive stars -- known as the Trapezium Cluster -- that is located just off the top right of the image. The strong and harsh ultraviolet radiation of the Trapezium cluster creates a hot, ionized environment in the upper right, and slowly erodes the Orion Bar away. Molecules and dust can survive longer in the shielded environment offered by the dense Bar, but the surge of stellar energy sculpts a region that displays an incredible richness of filaments, globules, young stars with disks and cavities. Image credit: NASA / ESA / CSA / PDRs4All ERS Team / Salomé Fuenmayor.

Webb Captures Breathtaking Images of Orion Nebula

Sep 12, 2022 by Enrico de Lazaro

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have delivered the most detailed images ever taken of the inner region of the Orion Nebula. The...

The unusual shape of the open cluster NGC 346 is partly due to stars and gas spiraling into the center of the cluster in a river-like motion; the red spiral superimposed on NGC 346 traces the movement of stars and gas toward the center; this spiraling motion is the most efficient way to feed star formation from the outside toward the center of the cluster. Image credit: NASA / ESA / Andi James, STScI.

Astronomers Find Spiraling Stars in NGC 346

Sep 8, 2022 by News Staff

Astronomers using the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s Very Large Telescope (VLT) and the NASA/ESA Hubble Space Telescope...

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