Search Results - "Kaaret, P."

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  1. 1

    Enhanced X-ray emission from Lyman break analogues and a possible LX-SFR-metallicity plane by Brorby, M, Kaaret, P, Prestwich, A, Mirabel, I F

    “…The source of energetic photons that heated and reionized the early Universe remains uncertain. Early galaxies had low metallicity and recent population…”
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    Journal Article
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    X-ray binary formation in low-metallicity blue compact dwarf galaxies by Brorby, M., Kaaret, P., Prestwich, A.

    “…X-rays from binaries in small, metal-deficient galaxies may have contributed significantly to the heating and reionization of the early Universe. We…”
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    Journal Article
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    Observations of Magnetospheric Solar Wind Charge Exchange by Ringuette, R., Kuntz, K. D., Koutroumpa, D., Kaaret, P., LaRocca, D., Richardson, J.

    Published in The Astrophysical journal (01-10-2023)
    “…Abstract The study of solar wind charge exchange (SWCX) emission is vital to both the X-ray astrophysics and heliophysics communities. SWCX emission…”
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  4. 4

    Effects of metallicity on high-mass X-ray binary formation by Ponnada, S, Brorby, M, Kaaret, P

    “…ABSTRACT The heating of the intergalactic medium in the early, metal-poor Universe may have been partly due to radiation from high-mass X-ray binaries (HMXBs)…”
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    Enhanced X-ray emission from candidate Lyman continuum emitting galaxies by Bluem, J, Kaaret, P, Prestwich, A, Brorby, M

    “…ABSTRACT X-ray binaries may have helped reionize the early Universe by enabling Lyman continuum escape. We analysed a set of eight local galaxies that are…”
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    A Disc-Dominated and Clumpy Circumgalactic Medium of the Milky Way Seen in X-Ray Emission by Kaaret, P, Koutroumpa, D, Kuntz, K D, Jahoda, K, Bluem, J, Gulick, H, Hodges-kluck, E, LaRocca, D M, Ringuette, R, Zajczyk, A

    Published in Nature astronomy (19-10-2020)
    “…The Milky Way galaxy is surrounded by a circumgalactic medium (CGM) that may play a key role in galaxy evolution as the source of gas for star formation and a…”
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  7. 7

    Revisiting the radio/X-ray flux correlation in the black hole V404 Cyg: from outburst to quiescence by Corbel, S., Koerding, E., Kaaret, P.

    “…We report results of Chandra X-ray and Very Large Array (VLA) radio observations of the Galactic accreting black hole V404 Cyg (GS 2023+338) in its quiescent…”
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    Rapid turn-on of a luminous X-ray source in the candidate Lyman continuum emitting galaxy Tol 0440-381 by Kaaret, P, Bluem, J, Prestwich, A H

    “…ABSTRACT Chandra observations of the nearby candidate Lyman continuum (LyC) emitting galaxy Tol 0440-381 show brightening of an X-ray source by at least a…”
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    THE 2015 DECAY OF THE BLACK HOLE X-RAY BINARY V404 CYGNI: ROBUST DISK-JET COUPLING AND A SHARP TRANSITION INTO QUIESCENCE by Plotkin, R. M., Miller-Jones, J. C. A., Gallo, E., Jonker, P. G., Homan, J., Tomsick, J. A., Kaaret, P., Russell, D. M., Heinz, S., Hodges-Kluck, E. J., Markoff, S., Sivakoff, G. R., Altamirano, D., Neilsen, J.

    Published in The Astrophysical journal (10-01-2017)
    “…ABSTRACT We present simultaneous X-ray and radio observations of the black hole X-ray binary V404 Cygni at the end of its 2015 outburst. From 2015 July…”
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  10. 10

    Observations of the Disk/Jet Coupling of MAXI J1820+070 during Its Descent to Quiescence by Shaw, A. W., Plotkin, R. M., Miller-Jones, J. C. A., Homan, J., Gallo, E., Russell, D. M., Tomsick, J. A., Kaaret, P., Corbel, S., Espinasse, M., Bright, J.

    Published in The Astrophysical journal (01-01-2021)
    “…Black hole X-ray binaries in the quiescent state (Eddington ratios typically 10−5) display softer X-ray spectra (photon indices Γ ∼ 2) compared to…”
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    A Search for the 3.5 keV Line from the Milky Way’s Dark Matter Halo with HaloSat by Silich, E. M., Jahoda, K., Angelini, L., Kaaret, P., Zajczyk, A., LaRocca, D. M., Ringuette, R., Richardson, J.

    Published in The Astrophysical journal (01-07-2021)
    “…Previous detections of an X-ray emission line near 3.5 keV in galaxy clusters and other dark-matter-dominated objects have been interpreted as observational…”
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  12. 12

    OPTICAL EMISSION OF THE ULTRALUMINOUS X-RAY SOURCE NGC 5408 X-1: DONOR STAR OR IRRADIATED ACCRETION DISK? by GRISE, F, KAARET, P, CORBEL, S, FENG, H, CSEH, D, TAO, L

    Published in The Astrophysical journal (01-02-2012)
    “…We obtained three epochs of simultaneous Hubble Space Telescope (HST)/Wide Field Camera 3 and Chandra observations of the ultraluminous X-ray source (ULX) NGC…”
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    The black hole candidate XTE J1752−223 towards and in quiescence: optical and simultaneous X-ray-radio observations by Ratti, E. M., Jonker, P. G., Miller-Jones, J. C. A., Torres, M. A. P., Homan, J., Markoff, S., Tomsick, J. A., Kaaret, P., Wijnands, R., Gallo, E., Özel, F., Steeghs, D. T. H., Fender, R. P.

    “…We present optical, X-ray and radio observations of the black hole transient (BHT) XTE J1752−223 towards and in quiescence. Optical photometry shows that the…”
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    A multi-wavelength view of distinct accretion regimes in the pulsating ultraluminous X-ray source NGC 1313 X-2 by Sathyaprakash, R, Roberts, T P, Grisé, F, Kaaret, P, Ambrosi, E, Done, C, Gladstone, J C, Kajava, J J E, Soria, R, Zampieri, L

    “…ABSTRACT NGC 1313 X-2 is one of the few known pulsating ultraluminous X-ray sources (PULXs), and so is thought to contain a neutron star that accretes at…”
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    Transition of an X-ray binary to the hard ultraluminous state in the blue compact dwarf galaxy VII Zw 403 by Brorby, M., Kaaret, P., Feng, H.

    “…We examine the X-ray spectra of VII Zw 403, a nearby low-metallicity blue compact dwarf (BCD) galaxy. The galaxy has been observed to contain an X-ray source,…”
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    HaloSat Observations of Heliospheric Solar Wind Charge Exchange by Ringuette, R., Koutroumpa, D., Kuntz, K. D., Kaaret, P., Jahoda, K., LaRocca, D., Kounkel, M., Richardson, J., Zajczyk, A., Bluem, J.

    Published in The Astrophysical journal (06-09-2021)
    “…X-ray emission from solar wind charge exchange (SWCX) produced in interplanetary space contaminates every astrophysical observation, regardless of the…”
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    A long-term X-ray monitoring of the ultraluminous X-ray source NGC 5408 X-1 with Swift reveals the presence of dips but no orbital period by Grisé, F., Kaaret, P., Corbel, S., Cseh, D., Feng, H.

    “…NGC 5408 X-1 is a well-studied ultraluminous X-ray source (ULX) that has been seen to emit in X-rays persistently above the Eddington limit of a stellar mass…”
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