Tag Archive for 'ALMA'

This artist’s conception shows the Jupiter-like protoplanet HD 169142b interacting with and heating nearby molecular gas, driving outflows seen in several emission lines, including those from shock-tracing molecules like SO and SiS, and the commonly seen 12CO and 13CO. Image credit: ALMA / ESO / NAOJ / NRAO / M. Weiss / AUI / NSF.

Astronomers Find Chemical Evidence for Planet Formation around HD 169142

Jun 28, 2023 by News Staff

Planets form in dusty, gas-rich circumstellar disks around young stars, while at the same time, the planet formation process alters the physical and chemical...

This image shows the Spiderweb protocluster, seen at a time when the Universe was only 3 billion years old. Image credit: ESO / Di Mascolo et al. / NASA / ESA / Hubble / H. Ford.

ALMA Detects Huge Reservoir of Hot Gas in Very Distant Galaxy Protocluster

Mar 29, 2023 by News Staff

The galaxy protocluster is question is forming around the recently-discovered Spiderweb galaxy (also known as MRC 1138-262 or PKS 1138-262), an object...

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...

SPT0418-47 is gravitationally lensed by a foreground galaxy, appearing in the sky as a near-perfect ring of light -- a so-called Einstein ring. Image credit: ALMA / ESO / NAOJ / NRAO / Rizzo et al.

Dusty, Chemically Mature Galaxy Spotted in Early Universe

Feb 28, 2023 by News Staff

The newly-discovered galaxy, SPT0418-SE, and its much larger companion, SPT0418-47, reside in a massive dark-matter halo with yet-to-be-discovered neighbors,...

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 composite image shows Messier 61, a spiral galaxy located 52.5 million light-years away in the constellation of Virgo. Image credit: ESO / ALMA / NAOJ / NRAO / PHANGS.

ESO Releases Stunning New Image of Messier 61

Feb 7, 2023 by Enrico de Lazaro

The new image of Messier 61, a spiral galaxy located in the constellation of Virgo, combines data taken at radio and visible wavelengths and is helping...

This image shows the distant galaxy GHZ2/GLASS-z12. Image credit: NASA / ESA / CSA / T. Treu, UCLA / NAOJ / T. Bakx, Nagoya University.

ALMA Confirms Discovery of Oxygen-Rich Galaxy in Very Early Universe

Jan 25, 2023 by News Staff

GHZ2/GLASS-z12, initially identified in the JWST GLASS survey, existed when the Universe was only 367 million years old (redshift z=12.117). This image...

This artist’s conception shows the galaxy merger and its two central black holes. Image credit: ALMA / ESO / NAOJ / NRAO / M. Weiss, NRAO, AUI & NSF.

UGC 4211’s Pair of Supermassive Black Holes is Closest to Colliding Ever Seen

Jan 11, 2023 by News Staff

While close together in cosmological terms at just 750 light-years apart, or 6x the black hole sphere of influence, the supermassive black holes in the...

This artist’s conception shows a zoomed in view of MWC 349A and its surrounding disk of gas and dust that are being shaped by the winds and high-speed jet. Image credit: ALMA / ESO / NAOJ / NRAO / M. Weiss, NRAO, AUI & NSF.

ALMA Spots Hidden Jet from Oddball Star MWC 349A

Jan 9, 2023 by News Staff

The jet observed by the Atacama Large Millimeter/submillimeter Array (ALMA) is ejecting material away from MWC 349A at a blistering 500 km per second (311...

The volcano-laced surface of Jupiter’s moon Io was captured in infrared by the Jovian Infrared Auroral Mapper (JIRAM) imager aboard NASA’s Juno spacecraft as it flew by at a distance of was about 80,000 km (50,000 miles) on July 5, 2022. Brighter spots indicate higher temperatures in this image. Image credit: NASA / JPL-Caltech / SwRI / ASI / INAF / JIRAM.

Trace Gas Detection Sheds New Light on Atmospheres of Jupiter and Its Volcanic Moon Io

Dec 28, 2022 by Natali Anderson

Using data from NSF’s Karl G. Jansky Very Large Array (VLA), the Atacama Large Millimeter/submillimeter Array (ALMA) and NASA’s Juno spacecraft, two...

This image shows Messier 66, an intermediate spiral galaxy located 31 million light-years away in the constellation of Leo. Image credit: ESO / PHANGS.

ESO Releases New Image of Spiral Galaxy Messier 66

Dec 13, 2022 by Enrico de Lazaro

This image of Messier 66 is a composite of separate exposures acquired by the Multi-Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope...

This composite image shows Messier 99, a grand design spiral galaxy located 42 million light-years away in the constellation of Coma Berenices. Image credit: ESO / PHANGS.

ESO Releases Incredible Image of Messier 99

Oct 24, 2022 by Enrico de Lazaro

This stunning image shows the well-defined arms of the grand design spiral galaxy Messier 99. This composite image shows Messier 99, a grand design spiral...

This artist’s illustration indicates where the modeling of the ALMA data predicts the hot spot to be and its orbit around Sagittarius A*. Image credit: ESO / M. Kornmesser / M. Wielgus / Event Horizon Collaboration.

ALMA Spots Bubble of Hot Gas in Orbit around Milky Way’s Central Black Hole

Sep 22, 2022 by News Staff

Sagittarius A*, the 4.3-million-solar-mass black hole at the center of our Milky Way Galaxy, was observed with the Atacama Large Millimeter/submillimeter...

An artist’s illustration of a protoplanet around LkCa 15; the protoplanet resides within dense rings of dust and gas that surround the star; material accumulates in a clump and arc-shape, about 60 degrees away from the protoplanet. Image credit: M. Weiss / Harvard & Smithsonian’s Center for Astrophysics.

ALMA Finds Evidence of Neptune-Mass Protoplanet around LkCa 15

Sep 15, 2022 by News Staff

LkCa 15, also known as IRAS 04363+2215, EPIC 247520207 or TIC 118681038, is a K5-type star with a mass of 1.2 solar masses. An artist’s illustration...

This artist’s conception shows the stream of gas and stars that were flung away from a massive galaxy during its merger with a smaller galaxy. Image credit: ALMA / ESO / NAOJ / NRAO / S. Dagnello, NRAO, AUI & NSF.

Massive Galaxy Strips Star-Forming Gas from Smaller Galaxy during Encounter

Aug 30, 2022 by News Staff

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) and the NASA/ESA Hubble Space Telescope have observed SDSS J144845.91+101010.5,...

An artist’s illustration of a protoplanetary disk; the insert displays carbon monoxide molecules in the ice phase. Image credit: M. Weiss / Harvard & Smithsonian’s Center for Astrophysics.

Astronomers Solve Mystery of Missing Gaseous Carbon Monoxide in Protoplanetary Disks

Aug 23, 2022 by News Staff

Carbon monoxide is ultra-bright and extremely common in protoplanetary disks, making it a prime target for astronomers. But a huge chunk of carbon monoxide...

Artist’s impression of an infant star still surrounded by a protoplanetary disk in which planets are forming. Image credit: L. Calçada / ESO.

ALMA Spots Circumplanetary Disk around Young Star AS 209

Aug 9, 2022 by News Staff

Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have detected the emission from 13CO — measure of the molecular gas distribution...

This artist’s conception shows the merger between a neutron star and another star (seen as a disk, lower left) which caused an explosion resulting in SGRB 211106A (white jet, middle), and left behind what astronomers now know to be one of the most luminous afterglows on record (semi-spherical shock wave mid-right); while dust in the host galaxy obscured most of the visible light (shown as colors), millimeter light from the event (depicted in green) was able to escape and reach ALMA. Image credit: ALMA / ESO / NAOJ / NRAO / M. Weiss, NRAO, AUI & NSF.

ALMA Looks at Neutron Star Merger in Millimeter Light

Aug 3, 2022 by News Staff

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have for the first time detected the millimeter afterglow of a short-duration...

Sagittarius B2 is a giant molecular cloud of gas and dust that is located about 390 light-years from the center of the Milky Way Galaxy. Sagittarius B2 is the bright orange-red region to the middle left of the image, which is centered on the Galactic center. Image credit: ESO / APEX / MSX / IPAC / NASA.

ALMA Detects Interstellar Propanol and Its Isomer in Milky Way’s Center

Jul 5, 2022 by Natali Anderson

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have detected two complex organic molecules — isopropanol (i-C3H7OH) and...

A schematic view of the history of the accretion disk and the flyby object: the three plots starting from the bottom left are snapshots from the numerical simulation, capturing the system right at the flyby event, 4,000 years after, and 8,000 years after, respectively; the top right image is from the ALMA observations, showing the disk with spirals and the two objects around it, corresponding to the system at 12,000 years after the flyby event. Image credit: Lu et al., doi: 10.1038/s41550-022-01681-4.

ALMA Images Spiral Protostellar Disk near Milky Way’s Center

Jun 21, 2022 by News Staff

Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have discovered a massive accretion disk with two spiral arms around a 32-solar-mass...

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