Low Mass X-ray Binaries and Metallicity Dependence: Story of Failures
arXiv:astro-ph/0509514 · doi:10.1086/498054
Abstract
Observations of galactic and extra-galactic globular clusters have shown that on average metal-rich clusters are ~3 times as likely to contain a bright X-ray source than their metal-poor counterparts. We propose that this can be explained by taking into account the difference in the stellar structure of main sequence donors with masses between ~0.85 Msun and ~1.25 Msun at different metallicities. Metal-poor main sequence stars in this mass range do not have an outer convective zone while metal-rich stars do. The absence of this zone turns off magnetic braking, a powerful mechanism of orbital shrinkage, leading to the failure of dynamically formed main sequence - neutron star binaries to start mass transfer or appear as bright low-mass X-ray binaries.
7 pages in ApJ style, 7 figures, accepted for publication in ApJ
References in corpus (4)
- The Evolution of Binary Fractions in Globular Clusters
- The ACS Virgo Cluster Survey III. Chandra and HST Observations of Low-Mass X-Ray Binaries and Globular Clusters in M87
- Formation of Ultracompact X-ray Binaries in Dense Star Clusters
- Three Additional Quiescent Low-Mass X-ray Binary Candidates in 47 Tucanae
Cited by in corpus (39)
- Compact Object Modeling with the StarTrack Population Synthesis Code
- Formation and evolution of compact binaries in globular clusters: II. Binaries with neutron stars
- Formation and evolution of compact binaries in globular clusters: I.Binaries with white dwarfs
- The Low-Mass X-ray Binary and Globular Cluster Connection in Virgo Cluster Early-type Galaxies: Optical Properties
- Faint X-ray Sources in the Globular Cluster Terzan 5
- Low Mass X-ray Binaries in 6 Elliptical Galaxies: Connection to Globular Clusters
- Probing the Formation of Low Mass X-ray Binaries in Globular Clusters and the Field
- Comparing GC and Field LMXBs in Elliptical Galaxies with deep Chandra and Hubble data
- Dynamical Formation of Millisecond Pulsars in Globular Clusters
- The binarity of Milky Way F,G,K stars as a function of effective temperature and metallicity
- Low-Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies. I. Chandra Observations
- Fermi Discovery of Gamma-ray Emission from the Globular Cluster Terzan 5
- Probing the GC-LMXB connection in NGC 1399: a wide-field study with HST and Chandra
- The Close Binary Properties of Massive Stars in the Milky Way and Low-Metallicity Magellanic Clouds
- Another thread in the tapestry of stellar feedback: X-ray binaries
- The evolution of the binary population in globular clusters: a full analytical computation
- A {\it Chandra} Survey of Milky Way Globular Clusters I: Emissivity and Abundance of Weak X-ray Sources
- The Origin of Gamma-Rays from Globular Clusters
- Metallicity Effect on LMXB Formation in Globular Clusters
- The Fundamental Plane of Gamma-ray Globular Clusters
- A systematic study of low mass X-ray binaries in the M31 globular cluster system
- X-ray Spectral Identification of Three Candidate Quiescent Low-Mass X-ray Binaries in the Globular Cluster NGC 6304
- Field and Globular Cluster LMXBs in NGC 4278
- The radial distribution of X-ray Binaries and Globular Clusters in NGC 4649 and their relation with the local stellar mass density
- Spatial distribution of luminous X-ray binaries in spiral galaxies
- Gamma-ray emission from globular clusters
- Low-Mass X-ray Binaries and Globular Clusters in Early-Type Galaxies. II. Globular Cluster Candidates and their Mass-Metallicity Relation
- Chandra Observations of the X-ray Point Source Population in NGC 4636
- On the origin of the metallicity dependence in dynamically formed extragalactic low-mass X-ray binaries
- Numerical modelling of gamma-ray emission produced by electrons originating from the magnetospheres of millisecond pulsars in globular clusters
- Gamma-ray emission from high Galactic latitude globular clusters
- The Luminosity Function of Low Mass X-Ray Binaries in the Globular Cluster System of NGC 1399
- Globular clusters hosting intermediate-mass black-holes: no mass-segregation based candidates
- Compact objects in globular clusters
- Stacking Star Clusters in M51: Searching for Faint X-Ray Binaries
- Neutron Stars and Black Holes in Star Clusters
- Evolution of binaries with compact objects in globular clusters
- An excess of low-mass X-ray binaries in the outer halo of NGC 4472
- Clues to Globular Cluster Evolution from Multiwavelength Observations of Extragalactic Systems