Black Holes and Neutron Stars in Nearby Galaxies: Insights from NuSTAR

Vulic, N ; Hornschemeier, A E ; Wik, D R ; Yukita, M ; Zezas, A ; Ptak, A F ; Lehmer, B D ; Antoniou, V ; Maccarone, T J ; Williams, B F(Washington Univ, Dept of Astronomy, Seattle, WA, United States)

关键词: BLACK HOLES (ASTRONOMY);    NEUTRON STARS;    GALAXIES;    STELLAR MASS;    X RAY BINARIES;    STAR FORMATION RATE;    SPECTROSCOPIC TELESCOPES;    X RAY ASTROPHYSICS FACILITY;    XMM-NEWTON TELESCOPE;    LUMINOSITY;    POINT SPREAD FUNCTIONS;    GOODNESS OF FIT;    ENERGY BANDS;    X RAYS;    POINT SOURCES;    SPACEBORNE TELESCOPES;    PULSARS;    X RAY SOURCES;    COMPARISON;    MILKY WAY GALAXY;   

RP-ID  :  GSFC-E-DAA-TN66572,GSFC-E-DAA-TN66100

学科分类：天体物理学

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

Nearby galaxy surveys have long classified X-ray binaries (XRBs) by the mass category of their donor stars (high-mass and low-mass). The NuSTAR (Nuclear Spectroscopic Telescope Array) observatory, which provides imaging data at E greater than 10 keV (kiloelectronvolts), has enabled the classification of extragalactic XRBs by their compact object type: neutron star (NS) or black hole (BH). We analyzed NuSTAR/Chandra/XMM-Newton observations from a NuSTAR-selected sample of 12 galaxies within 5 Mpc (megaparsecs) having stellar masses (M (sub asterisk)) 10 (sup 7-11) solar masses and star formation rates (SFRs) approximately 0.01-15 solar masses per year. We detected 128 NuSTAR sources to a sensitivity of 10 (sup 38) ergs per second. Using NuSTAR color-intensity and color-color diagrams we classified 43 of these sources as candidate NSs and 47 as candidate BHs. We further subdivide BHs by accretion states (soft, intermediate, and hard) and NSs by weak (Z/Atoll) and strong (accreting pulsar) magnetic field. Using eight normal (Milky Way-type) galaxies in the sample, we confirm the relation between the SFR and galaxy X-ray point source luminosity in the 4-25 and 12-25 keV energy bands. We also constrained galaxy X-ray point source luminosity using the relation L (sub X) equals M(sub asterisk) plus Beta SFR, finding agreement with previous work. The X-ray luminosity function (XLF) of all sources in the 4-25 and 12-25 keV energy bands matches the alpha = 1.6 slope for high-mass XRBs. We find that NS XLFs suggest a decline beginning at the Eddington limit for a 1.4 solar mass NS, whereas the BH fraction shows an approximate monotonic increase in the 4-25 and 12-25 keV energy bands. We calculate the overall ratio of BH to NS to be approximately 1 for 4-25 keV and approximately 2 for 12-25 keV.