T Coronae Borealis (T CrB), nicknamed the Blaze Star, is a binary star and a recurrent nova about 3,000 light-years (920 pc) away in the constellation Corona Borealis. [10] It was first …

2023年3月14日 · T CrB is one of the most-famous and brightest novae known, and is a recurrent nova with prior eruptions in 1866 and 1946 that peak at V = 2.0. I have constructed light …

Tau Coronae Borealis, Latinized from τ Coronae Borealis, is a possible astrometric and spectroscopic binary star system in the northern constellation of Corona Borealis. It is visible …

2024年6月12日 · The crown’s brightest star is Alpha (α) CrB, at magnitude 2.2 — about as bright as T CrB will appear in outburst. From there, look east down the crown’s curve, passing the …

北冕座T是一個 聯星系統，包含一顆巨大的低溫恆星和一顆緻密的高溫恆星。 主星是一顆表面溫度較低的 紅巨星，它正在將物質轉移到炙熱的伴星上。 熾熱的伴星全部隱藏在來自紅巨星的密 …

北冕座T（T CrB）非正式的称为“博雷兹星（the Blaze Star），是北冕座的一颗再发新星。 通常视星等为10，但在1866年和1946年曾经有过两次爆发，视星等达到了2.0，此外它在1217年10 …

T Coronae Borealis (T CrB) is a known recurrent nova with the next, long-anticipated explosion expected in early 2024. The 2024 nova eruption prediction is based on the approximately 80 …

The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

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Tau Coronae Borealis (τ CrB) is a spectral class K0III-IV star of magnitude 4.73 located in the constellation Corona Borealis. τ CrB is one of the brighter stars in Corona Borealis and can be …