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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 görüntüleme • 15 gün önce •via X (Twitter)

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NASA Universe profil fotoğrafı
NASA Universe15 gün önce

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:

Lightning Communications /\⚡/\ profil fotoğrafı
Lightning Communications /\⚡/\15 gün önce

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

ArchAngel profil fotoğrafı
ArchAngel15 gün önce

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

Interesting Radar profil fotoğrafı
Interesting Radar15 gün önce

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

Lady Jane profil fotoğrafı
Lady Jane15 gün önce

@JAXA_en @NASA @esa ♥️

Tamagochi Tg profil fotoğrafı
Tamagochi Tg15 gün önce

@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.

QuarkWino profil fotoğrafı
QuarkWino15 gün önce

@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.

MOON X profil fotoğrafı
MOON X15 gün önce

@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.

William Warden🇺🇸🗽 profil fotoğrafı
William Warden🇺🇸🗽15 gün önce

@JAXA_en @NASA @esa Nice artist conception animation.

Luca profil fotoğrafı
Luca15 gün önce

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

Myma profil fotoğrafı
Myma15 gün önce

@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

Vinicius Tostes profil fotoğrafı
Vinicius Tostes15 gün önce

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

Jon Burke profil fotoğrafı
Jon Burke15 gün önce

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

Symplectic profil fotoğrafı
Symplectic15 gün önce

@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.

Julio Ruiz profil fotoğrafı
Julio Ruiz15 gün önce

@JAXA_en @NASA @esa Beautiful 👏

ईमानदार आयकर दाता profil fotoğrafı
ईमानदार आयकर दाता15 gün önce

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

Unseen Light profil fotoğrafı
Unseen Light15 gün önce

@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:

Terrence profil fotoğrafı
Terrence15 gün önce

@JAXA_en @NASA @esa .

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