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AM Canum Venaticorum (AM CVn) stars belong to a class of ultra-compact, short period binaries with spectra dominated largely by helium.
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Nelemans G., 2005, in Hameury J.-M., Lasota J.-P., eds, The Astrophysics of Cataclysmic Variables and Related Objects Vol. 330 of Astronomical Society of the Pacific Conference Series, AM CVn stars. p. 27
2005
Cited alongside, same era.
Marsh T. R., Dhillon V. S., Littlefair S. P., Groot P. J., Hakala P., Nelemans G., Ramsay G., Roelofs G. H. A., Steeghs D., 2007, in Napiwotzki R., Burleigh M. R., eds, 15th European Workshop on White Dwarfs Vol. 372 of Astronomical Society of the Pacific Conference Series, SDSS J0926+3624, the First Eclipsing AM CVn Star, as Seen with ULTRACAM. p. 431
2007
Cited alongside, same era.
Ramsay G., Brocksopp C., Groot P. J., Hakala P., Lehto H., Marsh T. R., Napiwotzki R., Nelemans G., Potter S., Slee B., Steeghs D., Wu K., 2007, in Napiwotzki R., Burleigh M. R., eds, 15th European Workshop on White Dwarfs Vol. 372 of Astronomical Society of the Pacific Conference Series, Recent Observational Progress in AM CVn Binaries. p. 425
2007
Cited alongside, same era.
Later among the works it cites.
Levitan D. B., 2013, PhD thesis, California Institute of Technology
2013
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Mazin B. A., Meeker S. R., Strader M. J., Szypryt P., Marsden D., van Eyken J., Duggan G., Ulbricht G., Johnson M., Bumble B., O’Brien K., Stoughton C., 2013, PASP
2013
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