scispace - formally typeset
Search or ask a question

Which newly deployed telescope is going to help us understand the formation of stars better than ever before? 

Answers from top 7 papers

More filters
Papers (7)Insight
A telescope sensitive to mm radiation can therefore be used to observe nebulas in which stars are on the verge of forming.
With the proposed adaptive optics system, this new telescope is expected to resolve diffraction limited images, approximately an order of magnitude better than present seeing.
These findings will help to constrain the formation of massive stars.
The finding of a significant number of newly identified early-type star candidates at the Galactic center suggests that young, massive stars can be found throughout the entire cluster which may require us to modify existing theories for star formation at the Galactic center.
The presence of such a star within W51 shows that star formation has been underway for at least 3 Myr, while the formation of massive O stars is still on going.
Open accessJournal ArticleDOI
Jan Brand, J. G. A. Wouterloot 
35 Citations
The combination of old and recent activity implies that star formation has been going on for at least 20 Myr, which is difficult to understand considering the location of this object, where external triggers are either absent or weak, compared to the inner Galaxy.
Regardless of the star formation method, it appears certain that this group of stars is a coeval formation of various mass stars.

Related Questions

What is the current understanding of the Alpha Centauri system's formation and evolution?4 answersThe current understanding of the Alpha Centauri system's formation and evolution is that it likely formed as a triple system, with Proxima Centauri in a loosely bound orbit around the Alpha Centauri binary. The system's dynamics have been influenced by the Galactic tide and stellar encounters, which may have led to the capture of Proxima Centauri by the binary. The formation of planets within the system is plausible, with simulations suggesting that two or more terrestrial planets could exist around either Alpha Centauri A or B, within a region up to approximately 2 au. The presence of gas may facilitate planet formation. The age of the Alpha Centauri system is estimated to be around 5.3 billion years. Further research and improvements in data and models are needed to fully understand the system's history and its impact on the habitability of planets like Proxima b.
Last advancement's in Telescopes technology in year 2023?4 answersThe advancements in telescope technology in 2023 include the completion of a strategic change for the scientific use of the William Herschel Telescope (WHT) and the Isaac Newton Telescope (INT) at the Isaac Newton Group of Telescopes. The WHT will commission the WEAVE multi-fibre spectrograph and launch science surveys, offering 30% of the available time as open time. Additionally, the INT is being modernized and will operate as a robotic telescope, with an average of 40% of the time offered as open time. These advancements in telescope technology aim to improve the scientific applicability of adaptive optics (AO) and address technical challenges for future extremely large telescopes. The development of robotic telescopes, such as the 1.2-m MONET/South telescope and the 0.5-m vacuum tower telescope, also contributes to advancements in telescope technology.
What evidence do we have for star formation?7 answers
What is the name of ISRO new robot that will go to space next?8 answers
Where in the Milky Way do we see star formation happening?6 answers
Which part of our galaxy formed first since it has the oldest stars?6 answers

See what other people are reading

Hadoop applied to sky surveys
5 answers
Hadoop has been successfully applied to sky surveys, particularly in handling massive astronomical data streams. The use of Hadoop, a distributed computing technology, has enabled the efficient processing of large datasets generated by astronomical surveys like the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) and the Sloan Digital Sky Survey (SDSS). By leveraging the MapReduce paradigm within Hadoop, researchers have been able to implement scalable image-processing pipelines for tasks such as image coaddition, anomaly detection, classification, and moving object tracking in real-time. Furthermore, Hadoop's ability to partition data among worker nodes and schedule processing workloads in parallel has significantly enhanced the efficiency of analyzing astronomical data, paving the way for more advanced studies in the field of astronomy.
What are the interesting theories of all life connected at energy level ?
5 answers
Life is intricately connected at an energy level through various fascinating theories proposed in scientific literature. One theory suggests that life is a process where energy flows and diffuses, solidifying into semi-solid structures using DNA as a blueprint and proteins as basic units. Another intriguing concept highlights how virtually all atoms in living beings originate from stars across galaxies, while humans continuously generate nuclei through radioactive decay. Additionally, consciousness is hypothesized to emerge at a cellular level through quantum energy, utilizing electromagnetic radiation for communication within and across organisms. Furthermore, the flow of energy from the sun through plants to breathing animals powers not only physical functions but also thoughts, feelings, and consciousness, emphasizing the vital role of energy in connecting mind and body. These theories collectively underscore the profound interconnectedness of all life forms through energy dynamics.
How do ism filaments form?
5 answers
ISM filaments form due to the interplay of turbulence, magnetic fields, and ion-neutral friction. Turbulence induces strain, aligning filaments preferentially with the flow's stretch. Ion-neutral friction, or ambipolar diffusion, affects filament sizes by preventing small-scale compressions, leading to broader and more massive structures in non-ideal MHD simulations. In simulations of cloud formation by colliding flows, gravitational collapse of the cloud initiates filament formation, with gas flowing from the cloud to clumps within the filaments, creating long-lived flow features. The filaments are sustained by accretion from the environment and onto the clumps, showcasing a hierarchical nature with varying mass and density profiles, resembling observed characteristics in the interstellar medium.
What is age?
5 answers
AGE, or aging, refers to the process of biological changes leading to a decline in functions and an increased risk of death. It involves molecular-level alterations due to cellular dysfunction. The study of aging often involves model organisms like the naked mole-rat, which offers unique characteristics for research. Various theories highlight the impact of regulatory systems, such as hormonal regulation by growth hormone, on the aging process. Definitions of aging emphasize factors like persistent decline in fitness components due to internal physiological deterioration, and the study of linguistic units representing the concept of age in modern English language further enriches the understanding of this universal phenomenon. Aging is a fundamental aspect experienced by all living organisms, including humans, affecting bodily functions and overall health.
What is the significance of radio to UV SED modeling in understanding the properties of Infrared bright galaxies?
4 answers
Radio to UV SED modeling is significant in understanding the properties of Infrared bright galaxies. By simultaneously fitting the spectral energy distributions (SEDs) from radio to UV wavelengths, researchers can disentangle the emission between star formation (SF) and active galactic nuclei (AGN) in galaxies. This approach becomes particularly important for composite AGN/SF galaxies, which make up a significant portion of IR samples. Additionally, incorporating radio continuum measurements in SED fitting allows for improved accuracy in determining star formation rates and dust luminosities of galaxies. The radio SEDs can provide information about synchrotron emission and free-free absorption, shedding light on the presence of AGN and the energy balance between dust attenuation and emission. Therefore, radio to UV SED modeling is a valuable tool for studying the properties and contributions of AGN and SF in Infrared bright galaxies.
Amiga research operating system foreigh
4 answers
The AMIGA research project focuses on the development and implementation of a ground array system for the Pierre Auger Observatory. It consists of buried particle counters that provide measurements of the muon content in cosmic ray showers. The system utilizes an embedded control and data acquisition system to centrally manage and monitor the detectors. This system has been tested and proven to be reliable and stable, and it is being deployed in the production phase of the project. The research also involves the study of the physical conditions and distribution of metals in the circumgalactic medium (CGM) of the Andromeda galaxy using ultraviolet observations from the Hubble Space Telescope. The study reveals the presence of Si III and O VI ions in the CGM, with near unity covering factors maintained at large distances from the galaxy.
What is the sensivity level of terrebeldes stroemi?
4 answers
The sensitivity level of terrebeldes stroemi is not mentioned in any of the provided abstracts.
What are the best sources of K2?
4 answers
The best sources of vitamin K2 are fermented soybean products, fermented milk-based products such as cheese and soured milk, animal organs, meat, fish, and eggs. These sources contain ample amounts of menaquinones, specifically menaquinone-7 (MK-7) and menaquinone-4 (MK-4). Fermented vegetable products also contain menaquinones, with menaquinone-7 (MK-7) being the most abundant. Additionally, certain strains of lactic acid bacteria (LAB), such as Lactococcus lactis, have the capacity to produce long-chain vitamin K2 during fermentation processes. The production of vitamin K2 in LAB can be influenced by factors such as carbon sources and growth conditions. Overall, consuming fermented products and animal-based products can provide a significant dietary intake of vitamin K2.
How does the use of online ordering platforms affect the performance efficiency of businesses in the food industry?
4 answers
The use of online ordering platforms in the food industry has a significant impact on the performance efficiency of businesses. These platforms provide a convenient and accessible method for customers to place food orders, enhancing the process of receiving customer orders. They also create an ecosystem connecting restaurants and consumers, allowing restaurants to discover more potential consumers through platform resources. Additionally, online food delivery platforms have become popular, especially during the COVID-19 epidemic, and have influenced consumers' decision to order food online. The platforms' suitability and perceived ease of use play a crucial role in consumers' behavioral intentions and continued usage. However, the emergence of capital-monopolized platforms may distort market competition and impact the profit margins and survival space of restaurants, leading to increased food safety risks. Overall, online ordering platforms offer benefits in terms of convenience and customer reach, but their impact on businesses' performance efficiency depends on various factors, including platform suitability, competition dynamics, and government regulations.
Ism filaments formation mechanism
4 answers
Filament formation in the interstellar medium (ISM) is a topic of interest in recent research. Observations show that dense filaments are the sites of star formation, but the formation mechanism is not fully understood. Several mechanisms have been proposed, including shock waves and turbulence. Abe et al. conducted isothermal magnetohydrodynamics simulations and identified three different mechanisms for filament formation. They found that fast shock waves can create filaments regardless of turbulence and self-gravity, while slow shock waves induce filament formation through compressive flow. Ntormousi et al. explored the role of ion-neutral friction in filament formation and found that it affects the size and mass of filaments, but the observed filament thickness distribution was not fully reproduced in their simulations. In summary, filament formation in the ISM can be influenced by shock waves, turbulence, and ion-neutral friction, but further research is needed to fully understand the physics and mechanisms involved.
Warm global crysis?
5 answers
The abstracts provided do not contain any information related to a "warm global crisis."