By J. Mason
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Extra info for Astrophysics Update 2 - Topical and Timely Reviews on Astrophysics
Relativistic gravitational eﬀects, such as frame dragging (Bhattacharyya, Miller & Lamb 2004).
Moreover, neutron stars may contain states of matter not present anywhere else in the observable universe, for example, an exotic color-ﬂavor-locked (CFL), superﬂuid quark matter phase. Here, I discuss and review recent eﬀorts to measure neutron star masses and radii in order to use them as probes of fundamental physics. Such eﬀorts have focused on measurements of X-ray pulsation signals from both isolated and accreting neutron stars, as well as observations of the thermal emission from neutron star surfaces.
K. 2000, Molecular abundances in the atmosphere of the T dwarf Gl 229B, Astrophys. S. 2003, Non-equilibrium chemistry in the atmospheres of brown dwarfs. ASP Conf. Series IAU Symp. 211 on Brown Dwarfs (ed. N. 2001, Analysis of Keck HIRES spectra of early L-type dwarfs, Astrophys. D. 2002, Eﬀective temperatures of late L dwarfs and the onset of methane signatures, Astrophys. , & Chanover, N. 2001, L-band photometry of L and T dwarfs, Astrophys. , 556, L97-L101 Testi,L. , & Oliva, E. 45 micron spectra of L dwarfs: A near-infrared spectral classiﬁcation scheme for faint dwarfs, Astrophys.