Home » News & Blogs » Case for a Low Mass Black Hole
Bookmark and Share
Beyond Earthly Skies

Case for a Low Mass Black Hole

2 Jul 2015, 23:00 UTC
Case for a Low Mass Black Hole
(200 words excerpt, click title or image to see full post)

Neutron stars and black holes are two types of compact stellar remnants. The most massive known neutron star is about 2 times the Sun’s mass, while the least massive known black hole is about 4 times the Sun’s mass. There appears to be an absence of compact stellar remnants between 2 to 4 times the Sun’s mass. Neutron stars are unlikely to populate this mass gap since a neutron star more than twice the Sun’s mass is expected to gravitationally collapse into a black hole. However, black holes with 2 to 4 times the Sun’s mass are possible.Low mass X-ray binaries (LMXB) are a class of binary systems that are comprised of compact stellar remnants, either a neutron star or a black hole, that accretes material from a low mass companion star. Observations of a particular LMXB known as V1408 Aquilae show that the compact stellar remnant in this binary system is quite certainly a low mass black hole. Material stripped from the companion star forms an accretion disk around the black hole. Irradiation from the black hole’s accretion disk heats up one hemisphere of the companion star, resulting in a modulation in the light curve of the LMXB as ...

Latest Vodcast

Latest Podcast

Advertise PTTU

NASA Picture of the Day

Astronomy Picture of the Day