He had never known much of the Compact stars.

It is therefore another compact star, perhaps even a pulsar.

The result is one of the various types of compact star.

M31 is known to harbor a dense and compact star cluster at its very center.

In this case, compact stars would consist completely of quark matter all the way to their surface.

A compact star which is not a black hole may be called a degenerate star.

Pulsars are compact stars a few kilometres in diameter with masses around.

If the accretor is a compact star, an accretion disk may form.

Neither optical nor radio signals have been detected from the companion, and so it is also likely to be a compact star.

The end states are called compact stars.

The material in the disc slowly loses its angular momentum and falls into the compact star.

A white dwarf is a compact star that is no longer generating energy through nuclear fusion at its core.

Compact stars form the endpoint of stellar evolution.

Trapped modes would exist in extremely compact stars.

The accretion disc is drawn into the compact star by gravitational attraction with a large energy release (see Section 9.1).

Although compact stars may radiate, and thus cool off and lose energy, they do not depend on high temperatures to maintain their pressure.

It has been suggested that the observations of compact stars may also constrain the information about the high-density low-temperature region.

Gravitational collapse will usually occur on any compact star between 10 and 25 solar masses and produce a black hole.

For the astro-hadron physics, it has possibilities to explain the supernovae explosions and the structure of compact stars.

The other, donor, component usually fills its Roche lobe and therefore transfers mass to the compact star.

Eventually, given enough time (when we enter the so-called degenerate era of the universe), all stars will have evolved into dark, compact stars.

The types of compact stars are:

"Even among the needle habitats, whirling just above the compact star core, the potentials are many orders of magnitude too small.

In compact stars quark matter would occupy cubic kilometers and exist for millions of years, so the thermodynamic limit is appropriate.

The gravitational field of a compact star commonly pulls in gas from a companion star, thus radiation (especially X-ray) is emitted.