Search Results - "Pakull, M W"

A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source by Motch, C., Pakull, M. W., Soria, R., Grisé, F., Pietrzyński, G.

“…Ground-based and satellite observations show that the black hole in the ultraluminous X-ray source P13 has a mass of less than 15 times that of the Sun and…”
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The supergiant optical counterpart of ULX P13 in NGC 7793 by Motch, C., Pakull, M.W., Grisé, F., Soria, R.

“…We have identified the optical counterpart of the ULX source P13 in the nearby spiral galaxy NGC 7793. The object is a V ∼ 20.5 mag star, ten times brighter…”
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The face-on disc of MAXI J1836−194 by Russell, T. D., Soria, R., Motch, C., Pakull, M. W., Torres, M. A. P., Curran, P. A., Jonker, P. G., Miller-Jones, J. C. A.

“…We present Very Large Telescope optical spectra of the black hole candidate X-ray binary MAXI J1836−194 at the onset of its 2011 outburst. Although the…”
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A newly discovered double–double candidate microquasar in NGC 300 by Urquhart, R, Soria, R, Pakull, M W, Miller-Jones, J C A, Anderson, G E, Plotkin, R M, Motch, C, Maccarone, T J, McLeod, A F, Scaringi, S

“…We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova…”
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Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300 by McLeod, A F, Scaringi, S, Soria, R, Pakull, M W, Urquhart, R, Maccarone, T J, Knigge, C, Miller-Jones, J C A, Plotkin, R M, Motch, C, Kruijssen, J M D, Schruba, A

“…Abstract We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of…”
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Infrared identification of hard X-ray sources in the Galaxy by Nebot Gómez-Morán, A., Motch, C., Pineau, F.-X., Carrera, F. J., Pakull, M. W., Riddick, F.

“…The nature of the low- to intermediate-luminosity (L X ∼ 1032–34 erg s−1) source population revealed in hard band (2–10 keV) X-ray surveys of the Galactic…”
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Multiband counterparts of two eclipsing ultraluminous X-ray sources in M 51 by Urquhart, R, Soria, R, Johnston, H M, Pakull, M W, Motch, C, Schwope, A, Miller-Jones, J C A, Anderson, G E

“…Abstract We present the discovery and interpretation of ionized nebulae around two ultraluminous X-ray sources in M 51; both sources share the rare property of…”
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Optical Properties of the Ultraluminous X-Ray Source Holmberg IX X-1 and Its Stellar Environment by Grisé, F, Kaaret, P, Pakull, M. W, Motch, C

“…Holmberg IX X-1 is an archetypal ultraluminous X-ray source (ULX). Here we study the properties of the optical counterpart and of its stellar environment using…”
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Detection of an X-ray-ionized nebula around the black hole candidate binary LMC X-1 by PAKULL, M. W, ANGEBAULT, L. P

“…Optical spectra of the black hole candidate X-ray binary LMC X-1 reveal that the system is surrounded by an extended, highly ionized He III region, N159F,…”
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Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300 by McLeod, A. F, Scaringi, S, Soria, R, Pakull, M. W, Urquhart, R, Maccarone, T. J, Knigge, C, Miller-Jones, J. C. A, Plotkin, R. M, Motch, C, Kruijssen, J. M. D, Schruba, A

“…We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of kinematic…”
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The ultraluminous X-ray source bubble in NGC 5585 by Soria, R, Pakull, M W, Motch, C, Miller-Jones, J C A, Schwope, A D, Urquhart, R T, Ryan, M S

“…ABSTRACT Some ultraluminous X-ray sources (ULXs) are surrounded by collisionally ionized bubbles, larger and more energetic than supernova remnants: they are…”
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Multiband counterparts of two eclipsing ultraluminous X-ray sources in M 51 by Urquhart, R, Soria, R, Johnston, H. M, Pakull, M. W, Motch, C, Schwope, A, Miller-Jones, J. C. A, Anderson, G. E

“…We present the discovery and interpretation of ionized nebulae around two ultraluminous X-ray sources in M 51; both sources share the rare property of showing…”
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A newly discovered double-double candidate microquasar in NGC 300 by Urquhart, R, Soria, R, Pakull, M. W, Miller-Jones, J. C. A, Anderson, G. E, Plotkin, R. M, Motch, C, Maccarone, T. J, McLeod, A. F, Scaringi, S

“…We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova…”
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A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source by Motch, C, Pakull, M. W, Soria, R, Grisé, F, Pietrzyński, G

“…Nature, 514, 198-201 Most ultraluminous X-ray sources (ULXs) display a typical set of properties not seen in Galactic stellar-mass black holes (BHs): higher…”
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Neutral gas heating by X-rays in primitive galaxies: Infrared observations of IZw18 with Herschel by Lebouteiller, V, Pequignot, D, Cormier, D, Madden, S, Pakull, M. W, Kunth, D, Galliano, F, Chevance, M, Heap, S. R, Lee, M. -Y, Polles, F. L

“…A&A 602, A45 (2017) (abridged) The dominant thermal mechanisms in the neutral interstellar medium, which acts as a star-forming gas reservoir, are uncertain in…”
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LHG 83: Another outstanding X-ray binary in the LMC by Pakull, M.W., Ilovaisky, S.A., Chevalier, C.

“…The strongest X-ray point source, LHG 83, discovered in the Einstein survey of the LMC and not being associated with a nearby coronal type stellar emitter or…”
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Detection of an X-ray-ionized nebula around the black hole candidate binary LMC X-l by Pakull, M. W, Angebault, L. P

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Infrared identification of hard X-ray sources in the Galaxy by Gómez-Morán, A. Nebot, Motch, C, Pineau, F. -X, Carrera, F. J, Pakull, M. W, Riddick, F

“…The nature of the low- to intermediate-luminosity (Lx$\,\sim 10^{32-34}$ erg s$^{-1}$) source population revealed in hard band (2-10 keV) X-ray surveys of the…”
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CCD photometry of low mass X-ray binaries: LMCX-2, 1556-60 and 1957+11 by Motch, C., Chevalier, C., Ilovaisky, S.A., Pakull, M.W.

“…Preliminary results are presented from V-band CCD photometric observations of several low-mass X-ray binaries with faint optical counterparts that were…”
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The supergiant optical counterpart of ULX P13 in NGC7793 by Motch, C, Pakull, M. W, Grisé, F, Soria, R

“…We have identified the optical counterpart of the ULX source P13 in the nearby spiral galaxy NGC 7793. The object is a V ~ 20.5 mag star, ten times brighter…”
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