Large‐Scale Diffuse X‐Ray Emission from the Large Magellanic Cloud
نویسندگان
چکیده
منابع مشابه
Magnetic Field Structure of the Large Magellanic Cloud from Faraday Rotation Measures of Diffuse Polarized Emission
We present a study of the magnetic field of the Large Magellanic Cloud (LMC), carried out using diffuse polarized synchrotron emission data at 1.4 GHz acquired at the Parkes Radio Telescope and the Australia Telescope Compact Array. The observed diffuse polarized emission is likely to originate above the LMC disk on the near side of the galaxy. Consistent negative rotation measures (RMs) derive...
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Fourier transform power spectra of the distribution of neutral hydrogen emission in the Large Magellanic Cloud is approximately a power law over ∼ 2 decades in length. Power spectra in the azimuthal direction look about the same as the rectilinear spectra. No difference is seen between power spectra of single channel maps and power spectra of either the peak emission map or the integrated emiss...
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We have studied the variability of PSR J0529−6652, a radio pulsar in the Large Magellanic Cloud (LMC), using observations conducted at 1390 MHz with the Parkes 64 m telescope. PSR J0529−6652 is detectable as a single pulse emitter, with amplitudes that classify the pulses as giant pulses. This makes PSR J0529−6652 the second known giant pulse emitter in the LMC, after PSR B0540−69. The fraction...
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ژورنال
عنوان ژورنال: The Astrophysical Journal Supplement Series
سال: 2001
ISSN: 0067-0049,1538-4365
DOI: 10.1086/321799