Tag Archive for 'Protostar'

Optical (left) and infrared (right) image of NGC 346 in the Small Magellanic Cloud; the positions of the main ionizing sources of NGC 346, namely SSN 7 and SSN 9, are highlighted by red and green squares, respectively. Image credit: A. Nota, ESA & STScI / 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.

Two Massive Touching Stars Will Merge as Black Holes in 18 Billion Years, Astronomers Predict

Apr 27, 2023 by Enrico de Lazaro

SSN 7 is a so-called contact binary located in the Small Magellanic Cloud, a dwarf galaxy some 210,000 light-years away in the constellation of Tucana....

The left panel shows a three-color composite mosaic of NGC 346 combining Webb’s F277W (blue), F335M (green) and F444W (red) filters. The region is rich in structures of knots, arcs and filaments. Areas of bright pink and/or red emission are associated with clumpy star formation. The spatially resolved PAH emission excited by ultraviolet photons in green is brightest in regions corresponding to the edges of dense material, characteristic of a photodissociation region. Massive stars, stars belonging to the BS90 cluster (circled in green) and the Small Magellanic Cloud field population are also visible. The right panel shows a mosaic image from the F335M filter showing four different populations of stars: pre-main-sequence stars (blue circles), young stellar objects with Paα (orange diamonds), young stellar objects without Paα (red squares) and stars matched with the HST-PMS catalogue (purple stars). Image credit: Jones et al., doi: 10.1038/s41550-023-01945-7.

Webb Detects Planetary Ingredients in NGC 346

Apr 25, 2023 by Natali Anderson

Located in the Small Magellanic Cloud at a distance of roughly 200,000 light-years, NGC 346 is a prominent young cluster — roughly 3 million years...

This Hubble image shows NGC 1333, a reflection nebula located 1,000 light-years away in the northern constellation of Perseus. Image credit: NASA / ESA / STScI.

Hubble Captures NGC 1333 in Stunning 33rd Anniversary Image

Apr 20, 2023 by News Staff

This new photo of the reflection nebula NGC 1333 was taken in celebration of the 33rd anniversary of the launch of the NASA/ESA Hubble Space Telescope...

This image, captured by the Multi Unit Spectroscopic Explorer (MUSE) instrument on ESO’s Very Large Telescope (VLT), shows the young stellar object 244-440 in the Orion Nebula. Image credit: Kirwan et al. / ESO.

VLT Spots Spectacular Bipolar Jet from Young Stellar Object in Orion Nebula Cluster

Apr 18, 2023 by Natali Anderson

Astronomers using ESO’s Very Large Telescope have captured the most detailed image yet of the young stellar object 244-440 and the bipolar jet associated...

An artist’s impression of a gas-giant exoplanet. Image credit: Sci.News.

Low-Mass Stars are Able to Host Giant Jupiter-Like Exoplanets, Study Suggests

Mar 22, 2023 by News Staff

Gas giants, like other planets, form from protoplanetary disks of material around protostars. According to core accretion theory, they first form a core...

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...

This OmegaCAM/VST image shows IC 4701, an emission nebula located in the constellation of Sagittarius. Image credit: ESO / VPHAS+ team / Cambridge Astronomical Survey Unit.

VLT Survey Telescope Sees Newly-Born Stars in IC 4701

Mar 7, 2023 by Enrico de Lazaro

Astronomers using ESO’s VLT Survey Telescope have produced a spectacularly detailed image of the emission nebula IC 4701. This OmegaCAM/VST image shows...

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 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 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 Webb image shows the Pillars of Creation, a small star-forming region some 6,500 light-years away in the constellation of Serpens. Image credit: NASA / ESA / CSA / STScI / J. DePasquale, STScI / A. Pagan, STScI / A. M. Koekemoer, STScI.

Webb Team Releases Composite Image of Pillars of Creation

Dec 5, 2022 by Enrico de Lazaro

Astronomers have combined Webb’s near-infrared image with the mid-infrared image, setting the iconic Pillars of Creation ablaze with new details. This...

The protostar IRAS 04368+2557, shown in this Webb image, is embedded within LDN 1527, a cloud of material that is feeding its growth. Image credit: NASA / ESA / CSA / STScI / J. DePasquale, STScI.

Webb Sees Hourglass-Like Nebula around Young Protostar

Nov 16, 2022 by Enrico de Lazaro

Astronomers using the Near Infrared Camera (NIRCam) onboard the NASA/ESA/CSA James Webb Space Telescope have revealed new details surrounding the dark...

This image of Pillars of Creation includes mid-infrared observations from Webb’s MIRI instrument. Image credit: NASA / ESA / CSA / Webb / STScI / Joseph DePasquale, STScI / Alyssa Pagan, STScI.

Webb Sees Pillars of Creation in Mid-Infrared Light

Oct 30, 2022 by Enrico de Lazaro

The Webb team has released a high-resolution image of the Pillars of Creation captured by the Mid-Infrared Instrument (MIRI) on board the NASA/ESA/CSA...

This Hubble image shows NGC 1999, a reflection nebula some 1,350 light-years away in the constellation of Orion. The image also contains data from the OmegaCAM instrument on ESO’s VLT Survey Telescope. Image credit: NASA / ESA / Hubble / ESO / K. Noll.

Hubble Spies Mysterious Reflection Nebula

Oct 24, 2022 by Enrico de Lazaro

The Hubble science team has released an incredibly beautiful close-up shot of the reflection nebula NGC 1999. This Hubble image shows NGC 1999, a reflection...

This mosaic is composed of images covering the entire sky, taken by WISE as part of WISE’s 2012 All-Sky Data Release; by observing the entire sky, WISE can search for faint objects, like distant galaxies, or survey groups of cosmic objects. Image credit: NASA / JPL-Caltech / UCLA.

NEOWISE Mission Produces Time-Lapse Movie of Entire Sky

Oct 20, 2022 by News Staff

Using 18 all-sky maps produced by NASA’s Near-Earth Object Wide Field Infrared Survey Explorer (NEOWISE), astronomers have created what is essentially...

This image from Webb’s Near-Infrared Camera shows the Pillars of Creation. Image credit: NASA / ESA / CSA / STScI / Joseph DePasquale, STScI / Anton M. Koekemoer, STScI / Alyssa Pagan, STScI.

Webb Takes Close Look at Pillars of Creation

Oct 19, 2022 by News Staff

Protostars are the scene-stealers in this new image of the Pillars of Creation from the Near-Infrared Camera (NIRCam) instrument aboard the NASA/ESA/CSA...

This Hubble image shows IRAS 05506+2414, a young stellar object located over 12,000 light-years away in the constellation of Taurus. Image credit: NASA / ESA / Hubble / R. Sahai.

Hubble Looks at Very Young Protostar and Its Environment

Sep 19, 2022 by Enrico de Lazaro

Astronomers using the NASA/ESA Hubble Space Telescope have captured a stunning image of IRAS 05506+2414, an enigmatic stellar object surrounded by a shroud...

This 340-light-year-wide image from Webb’s Near-Infrared Camera (NIRCam) shows the Tarantula Nebula. Image credit: NASA / ESA / CSA / STScI / Webb ERO Production Team.

Webb Takes Close Look at Tarantula Nebula

Sep 6, 2022 by News Staff

The Tarantula Nebula, a turbulent star-birth region located in the Large Magellanic Cloud, hosts thousands of young and still-forming stars, many revealed...

This image, taken with the HAWK-I infrared instrument on ESO’s Very Large Telescope, shows the Sagittarius B1 region. Image credit: ESO / Nogueras-Lara et al.

Astronomers Detect Excess of Young Stars in Sagittarius B1

Aug 29, 2022 by Natali Anderson

Sagittarius B1, a region close to the center of our Milky Way Galaxy, hosts more than 100,000 solar masses of young stars. This image, taken with the...

A simulated star-forming region where massive stars destroy their parent cloud. Image credit: STARFORGE.

Star Formation is Self-Regulatory Process, New Research Suggests

Aug 8, 2022 by News Staff

Although star formation is one of the most fundamental processes of astrophysics, there is no widely accepted theory of star formation, despite decades...

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