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==Luminous supersoft X-ray sources==
Luminous super soft X-ray sources have a characteristic blackbody temperature of a few tens of eV (~20-100 eV)<ref name=Kahabka>{{ cite journal |author=Kahabka P |title=Supersoft X-ray sources |journal=Adv Space Res. |date=Dec 2006 |volume=38 |issue=12 |pages=2836–9 |url=http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6V3S-4MBT29S-2&_user=10&_origUdi=B6V3S-3YN948T-5&_fmt=high&_coverDate=12%2F31%2F2006&_rdoc=1&_orig=article&_acct=C000050221&_version=1&_urlVersion=0&_userid=10&md5=3a3d0440365be046b322ab561aae9230 |doi=10.1016/j.asr.2005.10.058 |bibcode=2006AdSpR..38.2836K}}</ref> and a bolometric luminosity of ~10<sup>38</sup> erg/s (below ~ 3 x 10<sup>38</sup> erg/s).<ref name=White>{{ cite journal |author=White NE, Giommi P, Heise J, Angelini L, Fantasia S |title=RX J0045.4+4154: A Recurrent Supersoft X-ray Transient in M31 |journal=Ap J Lett. |volume=445 |pages=L125 |url=http://lheawww.gsfc.nasa.gov/users/white/wgacat/apjl.html |doi=10.1086/187905|bibcode = 1995ApJ...445L.125W }}</ref><ref name=Kahabka/>
Apparently, luminous SSSs can have equivalent blackbody temperatures as low as ~15 eV and luminosities ranging from 10<sup>36</sup> to 10<sup>38</sup> erg/s.<ref name=KahabkaHeuvel>{{ cite journal |author=Kahabka P, van den Heuvel EPJ |title=Luminous Supersoft X-Ray Sources |journal=Ann Rev Astron Astrophys. |year=1997 |volume=35 |issue=1 |pages=69–100 |bibcode=1997ARA&A..35...69K |doi=10.1146/annurev.astro.35.1.69 }}</ref> The numbers of luminous SSSs in the disks of ordinary spiral galaxies such as the MW and M31 are estimated to be on the order of 10<sup>3</sup>.<ref name=KahabkaHeuvel/>
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