ფაილი:Millisecond pulsar and accretion disk - NASA animation (hi-res).ogv
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Millisecond_pulsar_and_accretion_disk_-_NASA_animation_(hi-res).ogv (ფაილის ზომა: 17,4 მბ, MIME ტიპი: application/ogg)
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English: Animation showing neutron star and accretion disk evolving into a millisecond pulsar, with magnetic fields.
The formation of a pulsar: A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. Deutsch: Animation: Die Entstehung eines Pulsars:
Ein Stern in einem Doppelsternsystem kollabiert zu einem Neutronenstern. Es beginnt Material von seinem Begleiter zu ihm zu strömen (Akkretion). Die einfallende Materie verursacht eine Beschleunigung und das Aussenden hoch-energetischer Strahlung. Schließlich ist ein Pulsar entstanden, der sich bis zu 1000 mal pro Sekunde dreht. Čeština: Animace vzniku pulsarů
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Millisecond pulsar and accretion disk - NASA animation (hi-res).ogv http://svs.gsfc.nasa.gov/vis/a010000/a010100/a010144/index.html |
| ავტორი | NASA (animator: Dana Berry) |
| სხვა ვერსიები |
File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv See also other versions on NASA pages |
File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv
File:Millisec xray pulsar H.jpg (still frame)
See also other versions on NASA pages
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This file was selected as the media of the day for 13 May 2011. It was captioned as follows:
English: Animation: the formation of a pulsar
A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. Other languages
Čeština: Animace vzniku pulsarů Deutsch: Animation: Die Entstehung eines Pulsars Ein Stern in einem Doppelsternsystem kollabiert zu einem Neutronenstern. Es beginnt Material von seinem Begleiter zu ihm zu strömen (Akkretion). Die einfallende Materie verursacht eine Beschleunigung und das Aussenden hoch-energetischer Strahlung. Schließlich ist ein Pulsar entstanden, der sich bis zu 1000 mal pro Sekunde dreht. English: Animation: the formation of a pulsar
A star in a binary star system has collapsed to a neutron star. It begins to gain material from its companion star (known as "accretion"). The infalling matter causes it to speed up and begin emitting high energy radiation, eventually forming a pulsar rotating at up to 1000 times a second. |
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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დააწკაპუნეთ თარიღზე/დროზე, რომ იხილოთ ფაილი ისე, როგორც ის მაშინ გამოიყურებოდა.
| თარიღი/დრო | განზომილებები | მომხმარებელი | კომენტარი | |
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| მიმდინარე | 16:14, 8 მაისი 2011 | (17,4 მბ) | wikimediacommons>FT2 | == {{int:filedesc}} == {{Information |Description ={{en|1=Animation showing neutron star and accretion disk evolving into a millisecond pulsar, with magnetic fields.}} |Source =Millisecond pulsar and accretion disk - NASA animation (hi-res). |
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