Английская Википедия:Bok globule
Шаблон:Infobox astronomical formationШаблон:Star formation In astronomy, Bok globules are isolated and relatively small dark nebulae, containing dense cosmic dust and gas from which star formation may take place. Bok globules are found within H II regions, and typically have a mass of about 2[1] to 50 solar masses contained within a region about a light year or so across (about [[Orders of magnitude (one cubic gigametre and greater)|Шаблон:Val]]).[2] They contain molecular hydrogen (H2), carbon oxides and helium, and around 1% (by mass) silicate dust. Bok globules most commonly result in the formation of double- or multiple-star systems.[3]
History
Bok globules were first observed by astronomer Bart Bok in the 1940s. In an article published in 1947, he and Edith F. Reilly hypothesized that these clouds were "similar to insect's cocoons" that were undergoing gravitational collapse to form new stars, from which stars and star clusters were born.[4]Шаблон:Failed verification This hypothesis was difficult to verify due to the observational difficulties of establishing what was happening inside a dense dark cloud that obscured all visible light emitted from within it. An analysis of near-infrared observations published in 1990 confirmed that stars were being born inside Bok globules.[5] Further observations have revealed that some Bok globules contain embedded warm sources,[2] some contain Herbig–Haro objects,[6] and some show outflows of molecular gas.[7] Millimeter-wave emission line studies have provided evidence for the infall of material onto an accreting protostar.[8] It is now thought that a typical Bok globule contains about 10 solar masses of material in a region about a light-year or so across, and that Bok globules most commonly result in the formation of double- or multiple-star systems.[5][9][10]
Bok globules are still a subject of intense research. Known to be some of the coldest objects in the natural universe, their structure and density remains somewhat a mystery. Methods applied so far have relied on column density derived from near-infrared extinction and even star counting in a bid to probe these objects further.
Bok globules that are irradiated by ultraviolet light from hot nearby stars exhibit stripping of materials to produce a tail. These types are called "cometary globules" (CG).[11]
Image gallery
-
Thackeray's Globules, a set of Bok globules in the H II region IC 2944, taken with the WFPC2 instrument on the Hubble Space Telescope
-
Bok globules located within the NGC 281 nebula (IC 1590 cluster)
-
Barnard 68, at a distance of only 410 light-years, is one of the nearest Bok globules. Its diameter is about Шаблон:Cvt (≈ 2 trillion km)
See also
References
External links
Шаблон:Star Шаблон:Star formation navbox Шаблон:Nebula Шаблон:Portal bar Шаблон:Authority control
- ↑ Шаблон:Cite web
- ↑ 2,0 2,1 Шаблон:Cite journal
- ↑ Шаблон:Cite conference
- ↑ Шаблон:Cite journal
- ↑ 5,0 5,1 Шаблон:Cite journal
- ↑ Шаблон:Cite journal
- ↑ Шаблон:Cite journal
- ↑ Шаблон:Cite journal
- ↑ Шаблон:Cite journal
- ↑ Шаблон:Cite conference
- ↑ Cometary globules. 1 Formation, evolution and morphology, B. Lefloch and B. Lazareff, 1994.
