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Home > Art, Film & Photography > O-Type Main Sequence Stars: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, SIGMA Orionis, Mu Columbae, HD 35619, Afgl 2591
O-Type Main Sequence Stars: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, SIGMA Orionis, Mu Columbae, HD 35619, Afgl 2591

O-Type Main Sequence Stars: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, SIGMA Orionis, Mu Columbae, HD 35619, Afgl 2591


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Chapters: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, Sigma Orionis, Mu Columbae, Hd 35619, Afgl 2591, Sigma Scorpii, Upsilon Sagittarii, Lh54-425, Omega Herculis. Source: Wikipedia. Pages: 41. Not illustrated. Free updates online. Purchase includes a free trial membership in the publisher's book club where you can select from more than a million books without charge. Excerpt: V838 Monocerotis (V838 Mon) is a red variable star in the constellation Monoceros about 20,000 light years (6 kpc) from the Sun. The star experienced a major outburst that was observed in early 2002. Originally believed to be a typical nova eruption, it was then realized to be something completely different. The reason for the outburst is still uncertain, but several theories have been put forward, including an eruption related to stellar death processes and a merger of a binary star or planets. On January 6, 2002, a previously unknown star was seen to brighten up in Monoceros, the Unicorn. Being a new variable star, it was designated V838 Monocerotis, the 838th variable star of Monoceros. The initial light curve resembled that of a nova, an eruption that occurs when enough hydrogen gas has accumulated on the surface of a white dwarf from its close binary companion. Therefore it was also designated Nova Monocerotis 2002. V838 Monocerotis reached maximum visual magnitude of 6.75 on February 6, 2002 after which it started to dim rapidly, as expected. However, in early March the star started to brighten again, this time mostly in infrared wavelengths. Yet another brightening in infrared occurred in early April after which the star returned to near its original brightness before the eruption, magnitude 15.6. The lightcurve produced by the eruption is unlike anything previously seen. The star brightened to about a million times solar luminosity ensuring that at the time of maximum V838 Monocerotis was one of the most luminous stars in the Mi...More: http://booksllc.net/?id=215164


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Product Details
  • ISBN-13: 9781156245248
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • Sub Title: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, SIGMA Orionis, Mu Columbae, HD 35619, Afgl 2591
  • Width: 229 mm
  • ISBN-10: 1156245249
  • Publisher Date: 15 Sep 2010
  • Binding: Paperback
  • Spine Width: 3 mm
  • Weight: 73 gr


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O-Type Main Sequence Stars: V838 Monocerotis, Ae Aurigae, Theta Orionis C, Ly Aurigae, SIGMA Orionis, Mu Columbae, HD 35619, Afgl 2591
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