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Membran 21.G - Eta Carinae (2) - Sister Anorexia (File, MP3)


Download Membran 21.G - Eta Carinae (2) - Sister Anorexia (File, MP3)
2011
Label: Jisatsuken - JSK 018 • Format: 3x, File MP3, EP 256kbps • Country: Bulgaria • Genre: Electronic • Style: Abstract, Ambient


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9 thoughts on “ Membran 21.G - Eta Carinae (2) - Sister Anorexia (File, MP3)

  1. Eta Carinae (η Carinae, abbreviated to η Car), formerly known as Eta Argus, is a stellar system containing at least two stars with a combined luminosity greater than five million times that of the Sun, located around 7, light-years (2, parsecs) distant in the constellation quaaccomtarganakal.brakparmosymsoulawestutelsulipetp.cously a 4th-magnitude star, it brightened in to become brighter than Rigel, marking the start of Constellation: Carina.

  2. Eta Carinae (η Carinae ili η Car) je zvjezdani sistem u sazviježđu Kobilica, udaljena do svjetlosnih godina od Sunca. Sistem sadrži najmanje dvije zvijezde od kojih je primarna η Car A je svijetla plava varijabilna zvijezda, koja je prvobitno imala oko masa Sunca, od kojih je izgubila najmanje Vreli supergigant zvijezda η Car B, težine otprilike 30 sunčevih masa.

  3. Eta Carinae is about 7, light-years from Earth and appears in the southern sky in the constellation Carina. At about times the mass of the Sun, Eta Carinae is a rare luminous blue variable star, a class that includes the brightest and most massive stars in the universe.

  4. Feb 02,  · Eta Carinae is one of the most remarkable stars in the heavens. This star was first cataloged by Edmond Halley in , as a star of fourth magnitude. Since, its brightness has varied in a most remarkable way: In , its brightness reached mag 2, and again fell to mag 4 in about It brightened again about and faded back to 4th.

  5. Sep 01,  · 2 December In the stellar system Eta Carinae suffered a violent explosion which caused it to become, in just a few decades, an amazingly beautiful nebula with two huge round blobs of material symmetrically distributed. For years astronomers have been looking for the cause of the explosion, and to explain the strange hourglass shape.

  6. We report the detection of the millimeter recombination lines H alpha, H alpha, H alpha, H Beta and H Beta towards Eta Carinae (Eta Car).

  7. Eta Carinae, the best-known Luminous Blue Variable (LBV), continues to confound astronomers as to what drives its historical outbursts and periodic changes. Is Eta Carinae a single star or a binary system In the past four years, determination of a spectroscopic year period led to coordinated observations throughout the spectrum that confirmed the periodicity.

  8. Eta Carinae’s Homunculus (little man in Latin) is a bipolar nebula, where we see a pair of roughly spherical lobes expanding at km/s, that are connected to each other near the central star ([6] and references therein). The equatorial plane orthogonal to the axis of the Homunculus contains ejected.

  9. May 20,  · Abstract: We evaluate the place of Eta Carinae amongst the class of luminous blue variables (LBVs) and show that the LBV phenomenon is not restricted to extremely luminous objects like Eta Car, but extends luminosities as low as log(L/Lsun) = - corresponding to initial masses ~25 Msun, and final masses as low as ~ Msun. We present a census of S Doradus variability, and discuss .

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