Showing posts with label HH 909A. Show all posts
Showing posts with label HH 909A. Show all posts

Friday, May 12, 2023

ESO telescope reveals hidden views of vast stellar nurseries

PR Image eso2307a
An infrared view of the L1688 region in Ophiuchus

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An infrared view of the Lupus 2 region

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An infrared view of the Lupus 3 region

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An infrared view of the HH 909 A object in Chamaeleon

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An infrared view of the IRAS 11051-7706 object in Chamaeleon

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An infrared view of the region around the Coronet star cluster

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The L1688 region in visible light

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The Lupus 3 region in visible light

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The Coronet region in visible light



Videos

Hidden views of vast stellar nurseries (ESOcast 262 Light)  



Using ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA), astronomers have created a vast infrared atlas of five nearby stellar nurseries by piecing together more than one million images. These large mosaics reveal young stars in the making, embedded in thick clouds of dust. Thanks to these observations, astronomers have a unique tool with which to decipher the complex puzzle of stellar birth.

In these images we can detect even the faintest sources of light, like stars far less massive than the Sun, revealing objects that no one has ever seen before,” says Stefan Meingast, an astronomer at the University of Vienna in Austria and lead author of the new study published today in Astronomy & Astrophysics. “This will allow us to understand the processes that transform gas and dust into stars.

Stars form when clouds of gas and dust collapse under their own gravity, but the details of how this happens are not fully understood. How many stars are born out of a cloud? How massive are they? How many stars will also have planets?

To answer these questions, Meingast’s team surveyed five nearby star-forming regions with the VISTA telescope at ESO’s Paranal Observatory in Chile. Using VISTA’s infrared camera VIRCAM, the team captured light coming from deep inside the clouds of dust. “The dust obscures these young stars from our view, making them virtually invisible to our eyes. Only at infrared wavelengths can we look deep into these clouds, studying the stars in the making,” explains Alena Rottensteiner, a PhD student also at the University of Vienna and co-author of the study.

The survey, called VISIONS, observed star-forming regions in the constellations of Orion, Ophiuchus, Chamaeleon, Corona Australis and Lupus. These regions are less than 1500 light-years away and so large that they span a huge area in the sky. The diameter of VIRCAM’s field of view is as wide as three full Moons, which makes it uniquely suited to map these immensely big regions.

The team obtained more than one million images over a period of five years. The individual images were then pieced together into the large mosaics released here, revealing vast cosmic landscapes. These detailed panoramas feature dark patches of dust, glowing clouds, newly-born stars and the distant background stars of the Milky Way.

Since the same areas were observed repeatedly, the VISIONS data will also allow astronomers to study how young stars move. “With VISIONS we monitor these baby stars over several years, allowing us to measure their motion and learn how they leave their parent clouds,” explains João Alves, an astronomer at the University of Vienna and Principal Investigator of VISIONS. This is not an easy feat, as the apparent shift of these stars as seen from Earth is as small as the width of a human hair seen from 10 kilometres away. These measurements of stellar motions complement those obtained by the European Space Agency’s Gaia mission at visible wavelengths, where young stars are hidden by thick veils of dust.

The VISIONS atlas will keep astronomers busy for years to come. “There is tremendous long-lasting value for the astronomical community here, which is why ESO steers Public Surveys like VISIONS,” says Monika Petr-Gotzens, an astronomer at ESO in Garching, Germany, and co-author of this study. Moreover, VISIONS will set the groundwork for future observations with other telescopes such as ESO’s Extremely Large Telescope (ELT), currently under construction in Chile and set to start operating later this decade. “The ELT will allow us to zoom into specific regions with unprecedented detail, giving us a never-seen-before close-up view of individual stars that are currently forming there,” concludes Meingast.



More Information

This research was presented in the paper “VISIONS: The VISTA Star Formation Atlas”, to appear in Astronomy & Astrophysics (doi: 10.1051/0004-6361/202245771)

The team is composed of Stefan Meingast (University of Vienna, Austria [Vienna]), João Alves (Vienna), Hervé Bouy (Université de Bordeaux, France [Bordeaux]), Monika G. Petr-Gotzens (European Southern Observatory, Germany [ESO]), Verena Fürnkranz (Max-Planck-Institut für Astronomie, Germany [MPIA]]), Josefa E. Großschedl (Vienna), David Hernandez (Vienna), Alena Rottensteiner (Vienna), Joana Ascenso (Universidade do Porto, Portugal [Porto]; Universidade de Lisboa, Portugal [Lisboa]), Amelia Bayo (ESO; Universidad de Valparaíso, Chile), Erik Brändli (Vienna), Anthony G. A. Brown (Leiden University, Netherlands), Jan Forbrich (University of Hertfordshire, UK [Hertfordshire]), Alyssa Goodman (Harvard-Smithsonian Center for Astrophysics, USA [CfA]), Alvaro Hacar (Vienna), Birgit Hasenberger (Vienna), Rainer Köhler (The CHARA Array of Georgia State University, USA), Karolina Kubiak (Lisboa), Michael Kuhn (Hertfordshire), Charles Lada (CfA), Kieran Leschinski (Vienna), Marco Lombardi (Università degli Studi di Milano, Italy), Diego Mardones (Universidad de Chile, Chile), Núria Miret-Roig (European Space Agency, European Space Research and Technology Centre, Netherlands [ESA]), André Moitinho (Lisboa), Koraljka Mužiiić (Porto; Lisboa), Martin Piecka (Vienna), Laura Posch (Vienna), Timo Prusti (ESA), Karla Peña Ramírez (Universidad de Antofagasta, Chile), Ronny Ramlau (Johannes Kepler University Linz, Austria; Johann Radon Institute for Computational and Applied Mathematics, Austria), Sebastian Ratzenböck (Vienna; Research Network Data Science at Uni Vienna), Germano Sacco (INAF – Osservatorio Astrofisico di Arcetri, Italy), Cameren Swiggum (Vienna), Paula Stella Teixeira (University of St Andrews, UK), Vanessa Urban (Vienna), Eleonora Zari (MPIA), and Catherine Zucker (Bordeaux).

The European Southern Observatory (ESO) enables scientists worldwide to discover the secrets of the Universe for the benefit of all. We design, build and operate world-class observatories on the ground — which astronomers use to tackle exciting questions and spread the fascination of astronomy — and promote international collaboration in astronomy. Established as an intergovernmental organisation in 1962, today ESO is supported by 16 Member States (Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom), along with the host state of Chile and with Australia as a Strategic Partner. ESO’s headquarters and its visitor centre and planetarium, the ESO Supernova, are located close to Munich in Germany, while the Chilean Atacama Desert, a marvellous place with unique conditions to observe the sky, hosts our telescopes. ESO operates three observing sites: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its Very Large Telescope Interferometer, as well as survey telescopes such as VISTA. Also at Paranal ESO will host and operate the Cherenkov Telescope Array South, the world’s largest and most sensitive gamma-ray observatory. Together with international partners, ESO operates ALMA on Chajnantor, a facility that observes the skies in the millimetre and submillimetre range. At Cerro Armazones, near Paranal, we are building “the world’s biggest eye on the sky” — ESO’s Extremely Large Telescope. From our offices in Santiago, Chile we support our operations in the country and engage with Chilean partners and society.



Link



Contacts:

Stefan Meingast
University of Vienna
Vienna, Austria
Email:
stefan.meingast@univie.ac.at

Juan Carlos Muñoz Mateos
ESO Media Officer
Garching bei München, Germany
Tel: +49 89 3200 6176
Email
: press@eso.org

Source: ESO/News


Monday, January 31, 2022

Hubble Examines a Star-Forming Chamaeleon

Chamaeleon Cloud I (Cha I)
Image Credit: NASA, ESA, K. Luhman and T. Esplin (Pennsylvania State University), et al., and ESO; Processing: Gladys Kober (NASA/Catholic University of America)

This NASA Hubble Space Telescope image captures one of three segments that comprise a 65-light-year wide star-forming region named the Chamaeleon Cloud Complex. The segment in this Hubble composite image, called Chamaeleon Cloud I (Cha I), reveals dusty-dark clouds where stars are forming, dazzling reflection nebulae glowing by the light of bright-blue young stars, and radiant knots called Herbig-Haro objects.

Herbig-Haro objects are bright clumps and arcs of interstellar gas shocked and energized by jets expelled from infant “protostars” in the process of forming. The white-orange cloud at the bottom of the image hosts one of these protostars at its center. Its brilliant white jets of hot gas are ejected in narrow torrents from the protostar’s poles, creating the Herbig-Haro object HH 909A.

The cross-like spikes around bright stars in the image occur when light waves from a very bright point source (like a star) bend around Hubble’s cross-shaped struts that support the telescope’s secondary mirror. As the light waves pass these struts, they coalesce on the other side, creating the bright, spikey starburst effect we see.

Hubble studied Cha I as part of a search for extremely dim, low-mass brown dwarfs. These “failed stars” lie somewhere in size between a large planet and a small star (10 to 90 times the mass of Jupiter), and do not have enough mass to ignite and sustain nuclear fusion in their cores. Hubble’s search found six new low-mass brown dwarf candidates that are helping astronomers better understand these objects.

This 315-million-pixel composite image is comprised of 23 observations made by Hubble’s Advanced Camera for Surveys. Gaps between those observations were filled by 20 Wide Field Planetary Camera 2 images. Any remaining gaps were filled with ground-based data from ESO’s VISTA VIRCAM. To download the full high-resolution version of this image, visit Hubble Captures Chamaeleon Cloud I.

Media Contact:

Claire Andreoli
NASA's Goddard Space Flight Center
301-286-1940

Editor: Andrea Gianopoulos

Source: NASA/Hubble


Friday, February 07, 2014

A nursery for unruly young stars

Credit: NASA & ESA.Acknowledgements: Kevin Luhman (Pennsylvania State University),  and Judy Schmidt

This striking new image, captured by the NASA/ESA Hubble Space Telescope, reveals a star in the process of forming within the Chamaeleon cloud. This young star is throwing off narrow streams of gas from its poles — creating this ethereal object known as HH 909A. These speedy outflows collide with the slower surrounding gas, lighting up the region.

When new stars form, they gather material hungrily from the space around them. A young star will continue to feed its huge appetite until it becomes massive enough to trigger nuclear fusion reactions in its core, which light the star up brightly.

Before this happens, new stars undergo a phase during which they violently throw bursts of material out into space. This material is ejected as narrow jets that streak away into space at breakneck speeds of hundreds of kilometres per second, colliding with nearby gas and dust and lighting up the region. The resulting narrow, patchy regions of faintly glowing nebulosity are known as Herbig-Haro objects. They are very short-lived structures, and can be seen to visibly change and evolve over a matter of years (heic1113) — just the blink of an eye on astronomical timescales.

These structures are very common within star-forming regions like the Orion Nebula, or the Chameleon I molecular cloud — home to the subject of this image. The Chameleon cloud is located in the southern constellation of Chameleon, just over 500 light-years from Earth. Astronomers have found numerous Herbig-Haro objects embedded in this stellar nursery, most of them emanating from stars with masses similar to that of the Sun. A few are thought to be tied to less massive objects such as brown dwarfs, which are "failed" stars that did not hit the critical mass to spark reactions in their centres.

A version of this image was entered into the Hubble's Hidden Treasures image processing competition by contestant Judy Schmidt.