WD 1337+705 is a star in the constellation Ursa Minor. Shining with an apparent magnitude of 12.8, it is white dwarf 0.59 times as massive as the Sun. It is 86.5 light-years distant from Earth. It has 3% of the Sun's luminosity. In 1997, Jay Holberg and colleagues discovered magnesium in its spectrum, which suggests that it has some low mass companion or accretion of material happening as the star's temperature is not hot enough for its intrinsic emission. Despite this, no direct evidence for a circumstellar disc, such as an infrared excess, has come to light.
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- WD 1337+705 (en)
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| - WD 1337+705 is a star in the constellation Ursa Minor. Shining with an apparent magnitude of 12.8, it is white dwarf 0.59 times as massive as the Sun. It is 86.5 light-years distant from Earth. It has 3% of the Sun's luminosity. In 1997, Jay Holberg and colleagues discovered magnesium in its spectrum, which suggests that it has some low mass companion or accretion of material happening as the star's temperature is not hot enough for its intrinsic emission. Despite this, no direct evidence for a circumstellar disc, such as an infrared excess, has come to light. (en)
- WD 1337+705 est une naine blanche de la constellation de la Petite Ourse. D'une magnitude apparente de 12,8, elle est distante de ∼86,5 a.l. (∼26,5 pc) de la Terre. Sa masse vaut 0,59 fois celle du Soleil mais sa luminosité n'est que de 3% celle du Soleil. (fr)
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| - WD 1337+705 est une naine blanche de la constellation de la Petite Ourse. D'une magnitude apparente de 12,8, elle est distante de ∼86,5 a.l. (∼26,5 pc) de la Terre. Sa masse vaut 0,59 fois celle du Soleil mais sa luminosité n'est que de 3% celle du Soleil. En 1997, Jay Holberg et ses associés ont détecté du magnésium dans son spectre, ce qui suggère qu'elle possède un compagnon de faible masse ou un disque d'accrétion, étant donné que la température de l'astre n'est pas suffisante pour que le magnésium soit issu d'une émission intrinsèque. Cependant, il n'existe à ce jour aucune évidence indiquant la présence d'un disque circumstellaire, comme par exemple un excès d'émission dans l'infrarouge. (fr)
- WD 1337+705 is a star in the constellation Ursa Minor. Shining with an apparent magnitude of 12.8, it is white dwarf 0.59 times as massive as the Sun. It is 86.5 light-years distant from Earth. It has 3% of the Sun's luminosity. In 1997, Jay Holberg and colleagues discovered magnesium in its spectrum, which suggests that it has some low mass companion or accretion of material happening as the star's temperature is not hot enough for its intrinsic emission. Despite this, no direct evidence for a circumstellar disc, such as an infrared excess, has come to light. (en)
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