Search Publications

Evidence of supercritical disc funnel radiation in X-ray spectra of SS 433
DOI: 10.1111/j.1365-2966.2009.15896.x Bibcode: 2010MNRAS.402..479M

Fabrika, S.; Medvedev, A.

We analysed the XMM-Newton spectra of SS433 using a standard model of adiabatically and radiatively cooling X-ray jets. The multitemperature thermal jet model reproduces the strongest observed emission line fluxes well. Fitting the He- and H-like iron line fluxes, we find that the visible blue jet base temperature is ~17 keV, the jet kinetic lumin…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
Evidence for a truncated accretion disc in the low-luminosity Seyfert galaxy, NGC 7213?
DOI: 10.1111/j.1365-2966.2010.17143.x Bibcode: 2010MNRAS.408..551L

Turner, T. J.; Porquet, D.; Reeves, J. N. +4 more

We present the broad-band 0.6-150keV Suzaku and Swift BAT spectra of the low-luminosity Seyfert galaxy, NGC 7213. The time-averaged continuum emission is well fitted by a single power law of photon index Γ = 1.75, and from consideration of the Fermi flux limit we constrain the high-energy cut-off to be 350keV < Ecut < 25MeV. Line …

2010 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 27
Estimating the masses of extra-solar planets
DOI: 10.1111/j.1365-2966.2010.17233.x Bibcode: 2010MNRAS.408.1606W

Dhillon, V. S.; Littlefair, S. P.; Collier Cameron, A. +2 more

All extra-solar planet masses that have been derived spectroscopically are lower limits since the inclination of the orbit to our line-of-sight is unknown except for transiting systems. In theory, however, it is possible to determine the inclination angle, i, between the rotation axis of a star and an observer's line-of-sight from measurements of …

2010 Monthly Notices of the Royal Astronomical Society
Hipparcos 26
X-ray spectroscopy of the hot gas in the M31 bulge
DOI: 10.1111/j.1365-2966.2010.16404.x Bibcode: 2010MNRAS.404.1879L

Wang, Q. Daniel; Liu, Jiren; Li, Zhiyuan +1 more

We present an X-ray spectroscopic study of the nuclear region of the M31 bulge, based on observations of the XMM-Newton Reflection Grating Spectrometers. The obtained high-resolution grating spectra clearly show individual emission lines of highly ionized iron and oxygen, which unambiguously confirm the presence of diffuse hot gas in the bulge, as…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
The quest for the Sun's siblings: an exploratory search in the Hipparcos Catalogue
DOI: 10.1111/j.1365-2966.2010.16921.x Bibcode: 2010MNRAS.407..458B

Brown, Anthony G. A.; Portegies Zwart, Simon F.; Bean, Jennifer

We describe the results of a search for the remnants of the Sun's birth cluster among stars in the Hipparcos Catalogue. This search is based on the predicted phase-space distribution of the Sun's siblings from simple simulations of the orbits of the cluster stars in a smooth Galactic potential. For stars within 100 pc, the simulations show that it…

2010 Monthly Notices of the Royal Astronomical Society
Hipparcos 26
Star formation history of KDG61 and KDG64 from spectroscopy and colour-magnitude diagrams
DOI: 10.1111/j.1365-2966.2010.16746.x Bibcode: 2010MNRAS.406.1152M

Makarova, Lidia; Makarov, Dmitry; Koleva, Mina +1 more

A study of two dE/dSph members of the nearby M81 group of galaxies, KDG61 and UGC5442 = KDG64, has been made. Direct Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) images and integrated-light spectra of 6-m telescope of Special Astrophysical Observatory of Russian Academy of Sciences have been used for quantitative star formation h…

2010 Monthly Notices of the Royal Astronomical Society
eHST 26
SAO RAS 6-m telescope spectroscopic observations of globular clusters in nearby galaxies
DOI: 10.1111/j.1365-2966.2010.16510.x Bibcode: 2010MNRAS.405..839S

Chandar, Rupali; Goudfrooij, Paul; Puzia, Thomas H. +2 more

We present the results of medium-resolution spectroscopy of 28 globular clusters (GCs) in six nearby galaxies of different luminosities and morphological types, situated in M33 (15 objects), M31 (three), IC10 (four), UGCA86 (four), Holmberg IX (one) and DDO71 (one) obtained at the Special Astrophysical Observatory 6-m telescope. Measurements of Li…

2010 Monthly Notices of the Royal Astronomical Society
eHST 26
Using the ROSAT catalogue to find counterparts for unidentified objects in the first Fermi/LAT catalogue
DOI: 10.1111/j.1365-2966.2010.17123.x Bibcode: 2010MNRAS.408..422S

Masetti, N.; Landi, R.; Malizia, A. +4 more

There are a total of 1451 gamma-ray emitting objects in the Fermi Large Area Telescope First Source Catalogue. The point source location accuracy of typically a few arcmin has allowed the counterparts for many of these sources to be found at other wavelengths, but even so there are 630 which are described as having no plausible counterpart at 80 p…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
Fading of the X-ray flux from the black hole in the NGC 4472 globular cluster RZ 2109
DOI: 10.1111/j.1745-3933.2010.00953.x Bibcode: 2010MNRAS.409L..84M

Kundu, Arunav; Zepf, Stephen E.; Maccarone, Thomas J. +1 more

We present the results of new X-ray observations of XMMU 122939.7+075333, the black hole (BH) in the globular cluster RZ 2109 in the Virgo cluster galaxy NGC 4472. A combination of non-detections and marginal detections in several recent Swift and Chandra observations show that the source has varied by at least a factor of 20 in the past 6 yr, and…

2010 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
H2 reformation in post-shock regions
DOI: 10.1111/j.1745-3933.2010.00871.x Bibcode: 2010MNRAS.406L..11C

Kristensen, L. E.; Cuppen, H. M.; Gavardi, E.

H2 formation is an important process in post-shock regions, since H2 is an active participant in the cooling and shielding of the environment. The onset of H2 formation therefore has a strong effect on the temperature and chemical evolution in the post-shock regions. We recently developed a model for H2

2010 Monthly Notices of the Royal Astronomical Society
ISO 25