AB Boötis
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AB Boötis, also known as Nova Boötis 1877 and occasionally Nova Comae Berenices 1877, is an object that may have undergone a
nova A nova (plural novae or novas) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star (hence the name "nova", which is Latin for "new") that slowly fades over weeks or months. Causes of the dramati ...
outburst in 1877. It was discovered by Friedrich Schwab at
Technische Universität Ilmenau The Technische Universität Ilmenau (''Ilmenau University of Technology'', TU Ilmenau) is a German public research university located in Ilmenau, Thuringia, central Germany. Founded in 1894, it has five academic departments (faculties) with abo ...
in 1877. He reported observing the star as a 5th
magnitude Magnitude may refer to: Mathematics *Euclidean vector, a quantity defined by both its magnitude and its direction *Magnitude (mathematics), the relative size of an object *Norm (mathematics), a term for the size or length of a vector *Order of ...
object, visible to the naked eye, on 14 nights during the period from 30 May 1877 through 14 July 1877. The star was lost, and despite several searches in subsequent years, no other 19th century observations of the nova were reported. Downes ''et al.'' estimate that Schwab's reported coordinates for the star may have had a precision no better than 1/2 degree. In 1971, A. Sh. Khatisov suggested that the star Schwab saw was BD +21°2606 (whose visual magnitude is 10.64 in the
Tycho-2 Catalogue The Tycho-2 Catalogue is an astronomical catalogue of more than 2.5 million of the brightest stars. Catalogue The astrometric reference catalogue contain positions, proper motions, and two-color photometric data for 2,539,913 of the brightes ...
, roughly 100 times fainter than the object Schwab reported), but that identification may be incorrect. In 1988 Downes and Szkody imaged the area around AB Boötis' reported position, to try to identify the nova in its quiescent state based on its color, but their search was unsuccessful. In 2000, Liu ''et al.'' published a spectrum of AB Boötis, which they describe as a cataclysmic variable (a class which includes novae), but they did not publish the coordinates of the star they examined, so exactly which star they observed is unclear. In 2020, Hoffmann and Vogt suggested that AB Boötis might be a re-appearance of a
guest star In show business, a guest appearance is the participation of an outsider performer (such as a musician or actor) in an event such as a music record or concert, show, etc., when the performer does not belong to the regular band, cast, or other ...
that Chinese astronomers saw near
Arcturus , - bgcolor="#FFFAFA" , Note (category: variability): , , H and K emission vary. Arcturus is the brightest star in the northern constellation of Boötes. With an apparent visual magnitude of −0.05, it is the third-brightest of th ...
in 203
BCE Common Era (CE) and Before the Common Era (BCE) are year notations for the Gregorian calendar (and its predecessor, the Julian calendar), the world's most widely used calendar era. Common Era and Before the Common Era are alternatives to the or ...
.


References

{{Stars of Boötes Novae Boötes 1877 in science Boötis, AB 18770530