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Peculiar high-speed X-ray jets associated with the 18 June 1999 limb flares have directly been observed with the soft X-ray
Telescope (SXT) aboard Yohkoh. The jets have a much shorter lifetime (within 200 s) and a much larger velocity (∼ 1700 km s−1) than the previously reported jets. Judged from their large velocity, the kinetic energy of the jets is approximately one
order of magnitude larger than the thermal energy content, which is far different from the jets previously reported by other
researchers. Here we present the preliminary results and discuss the particular features of the jets.
Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1013324126229 相似文献
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Minhwan Jang 《Astrophysics and Space Science》2001,275(3):209-215
Preliminary results from a pilot program to monitor the intranightoptical variability in Seyfert 2 galaxies are reported. This program is designed to test some of the prominent theoretical mechanismsproposed for the origin of optical microvariability in active galacticnuclei (AGN). Two out of 3 Seyfert 2 galaxies observed show evidence formicrovariations. This detection can provide important constraints forthe models utilizing discrete events on accretion disks. 相似文献
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Haingja Seo Sungwon Hwang Aeran Jung Ji Hyun Kim Joo Hyeon Kim Kap-Sung Kim Jinny Lee Minhwan Jang 《Icarus》2007,192(1):287-295
We have constructed synthetic solar spectra for the 2302-4800 cm−1 (2.08-4.34 μm) range, a spectral range where planetary objects mainly emit reflected sunlight, using ATMOS (Atmospheric Trace Molecule Spectroscopy)/Spacelab-3 and Atlas-3 spectra, of which resolution is 0.01 cm−1. We adopted Voigt line profiles for the modeling of line shapes based on an atlas of line identifications compiled by Geller [Geller, M., 1992. Key to Identification of Solar Features. A High-Resolution Atlas of the Infrared Spectrum of the Sun and the Earth Atmosphere from Space. NASA Reference Publ. 1224, vol. III. NASA, Washington, DC, pp. 1-22], who derived solar line positions and intensities from contaminated high-resolution solar spectra obtained by ATMOS/Spacelab-3. Because the ATMOS spectra in these wavelength ranges are compromised by absorption lines of molecules existing in Earth's high-altitude atmosphere and in the compartment of the spacecraft, the direct use of these high-resolution solar spectra has been inconvenient for the data reductions of planetary spectra. We compared the synthetic solar spectra with the ATMOS spectra, and obtained satisfactory fits for the majority of the solar lines with the exception of abnormal lines, which do not fit with Voigt line profiles. From the model fits, we were able to determine Voigt line parameters for the majority of solar lines; and we made a list of the abnormal lines. We also constructed telluric-line-free solar spectra by manually eliminating telluric lines from the ATMOS spectra and filling the gaps with adjacent continua. These synthetic solar spectra will be useful to eliminate solar continua from spectra of planetary objects to extract their own intrinsic spectral features. 相似文献
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This is a preliminary report of the continuing search for significant optical microvariability in a selected sample of radio-quiet
and radio-loud quasi-stellar objects (QSOs). Total of 24 Paloma-Green (PG) quasars are observed. Among them, 17 objects are
classified as radio-quiet and seven objects are classified radio-loud. In this classification, the ratio R, radio to optical
flux density, is required to be less than 1 in order to assure the objects are reasonably radio-quiet. Two out of 17 radio-quiet
QSOs and six out of eight radio-loud QSOs were microvariable. This apparent contrast in microvariations between radio-quiet
and radio-loud QSOs does not provide firm support for the theoretical model utilizing discrete events in accretion disks and
implies substantial support for models based on propagating shocks on relativistic jets as the likely process responsible
for producing most of the microvariations are observed in AGNs. 相似文献
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