. | . |
Age of NGC 6652 globular cluster specified by Staff Writers Kazan, Russia (SPX) May 06, 2020
Senior Research Associate Margarita Sharina (Special Astrophysical Observatory) and Associate Professor Vladislav Shimansky (Kazan Federal University) studied the globular cluster NGC 6652.4.05957 and found out that its age is close to 13.6 billion years, which makes it one of the oldest objects in the Milky Way. Globular clusters are mostly situated tens and hundreds of thousands of light years from Earth, and only the brightest stars in them can actually be studied. Margarita Sharina, a Kazan Federal University alumna, came up with the idea of researching the spectra of full star clusters several years ago. Together with Vladislav Shimansky, she developed Cluster, a special software package to model such spectra. During their joint work, the two scientists have determined fundamental characteristics of almost 40 globular clusters. In this paper, they analyzed the spectra of NGC 6652 obtained by the Cerro Tololo Observatory. The overall ratio of heavy elements in the cluster turned out to be unusually high. Furthermore, some anomalies in the ratio of several elements (carbon, nitrogen, sodium, magnesium, calcium, and titanium).
"For a long time, the consensus At the same time, its metallicity is rather high. The reason, hypothetically, is its unusual dynamics - the matter which formed the cluster has passed through the galactic disk multiple times and amassed the heavy elements synthesized there." Studying globular clusters with up to a million stars can help research the early stages of the Universe. During this past decade, many large telescopes have been observing galactic and extragalactic globular clusters - natural laboratories which facilitate the studies of stars and galaxies. Many more interesting discoveries are to be made after more data is deciphered, concludes Shimansky.
Beyond the Brim, Sombrero galaxy's halo suggests turbulent past Baltimore MD (SPX) Feb 21, 2020 Surprising new data from NASA's Hubble Space Telescope suggests the smooth, settled "brim" of the Sombrero galaxy's disk may be concealing a turbulent past. Hubble's sharpness and sensitivity resolves tens of thousands of individual stars in the Sombrero's vast, extended halo, the region beyond a galaxy's central portion, typically made of older stars. These latest observations of the Sombrero are turning conventional theory on its head, showing only a tiny fraction of older, metal-poor stars in t ... read more
|
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us. |