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For the first time, astronomers directly observed stellar wind flowing from a giant star onto its companion, causing powerful X-ray flares. Data from the XRISM telescope, which is led by JAXA(Japan Aerospace Exploration Agency) in partnership with NASA and with contributions from @ESA, revealed the cause. 🧵

50,952 просмотров • 15 дней назад •via X (Twitter)

Комментарии: 18

Фото профиля NASA Universe
NASA Universe15 дней назад

Outflows of gas from the giant star are captured by its pulsar companion, a dense, rapidly spinning stellar remnant. The flares, which last several days, occur twice each orbit when the pulsar passes through a dense stream of gas. Learn more:

Фото профиля Lightning Communications /\⚡/\
Lightning Communications /\⚡/\15 дней назад

@JAXA_en @NASA @esa Hi .. Reminds me of my photo's I took of the Sun years ago .. Flashing ..

Фото профиля ArchAngel
ArchAngel15 дней назад

@JAXA_en @NASA @esa I want to see 👀 real images not an artist conception. Astronomers can't 'directly observe' a concept! Ty

Фото профиля Interesting Radar
Interesting Radar15 дней назад

@JAXA_en @NASA @esa If those flares last several days, how long is the pulsar actually passing through that dense stream each time?

Фото профиля Lady Jane
Lady Jane15 дней назад

@JAXA_en @NASA @esa ♥️

Фото профиля Tamagochi Tg
Tamagochi Tg15 дней назад

@JAXA_en @NASA @esa That stellar wind must feel like a firehose to the face-makes me grateful my own feeding schedule is just me frantically tapping on a tiny screen. Check the header, my Tamagotchi is always hungry.

Фото профиля QuarkWino
QuarkWino15 дней назад

@JAXA_en @NASA @esa Stellar wind became the fuel. XRISM tracked the X-ray-emitting gas to the companion, finally revealing how a seemingly ordinary stellar wind can power million-degree plasma.

Фото профиля MOON X
MOON X15 дней назад

@JAXA_en @NASA @esa Stellar wind caught flowing onto a companion — XRISM making the invisible transfer visible. Glad JAXA, NASA, and ESA shared that first look in public.

Фото профиля William Warden🇺🇸🗽
William Warden🇺🇸🗽15 дней назад

@JAXA_en @NASA @esa Nice artist conception animation.

Фото профиля Luca
Luca15 дней назад

@JAXA_en @NASA @esa i am deaf history welcome vision

Фото профиля Myma
Myma15 дней назад

@JAXA_en @NASA @esa The system is BP Crucis, 13,000 light-years away, where the blue hypergiant Wray 977 loses ionised gas in a stellar wind that feeds the rapidly spinning neutron star pulsar GX 301-2 twice per 41.5-day orbit. Grok

Фото профиля Vinicius Tostes
Vinicius Tostes15 дней назад

@JAXA_en @NASA @esa @NASAUniverse what kind of star are those? The main and the companion one? Is the companion one a pulsar?

Фото профиля Jon Burke
Jon Burke15 дней назад

@JAXA_en @NASA @esa Fake artist rendition...

Фото профиля Symplectic
Symplectic15 дней назад

@JAXA_en @NASA @esa Really amazing how gravity turns the captured stellar wind into an energy source, heating the infalling gas until it glows in X-rays.

Фото профиля Julio Ruiz
Julio Ruiz15 дней назад

@JAXA_en @NASA @esa Beautiful 👏

Фото профиля ईमानदार आयकर दाता
ईमानदार आयकर दाता15 дней назад

@JAXA_en @NASA @esa How can wind "flow" in space, as in a vaccum? Kindly clarify

Фото профиля Unseen Light
Unseen Light15 дней назад

@JAXA_en @NASA @esa Those X-ray flares are ordinary gas lighting up as it hits a pulsar. Bright, and still the small piece. Most of a galaxy's mass never glows. More:

Фото профиля Terrence
Terrence15 дней назад

@JAXA_en @NASA @esa .

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