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In the hotter G-type stars, however, the lines of ionized calcium at 3968 and 3933 Å (the "H" and "K" lines) become much stronger than any other feature in the spectrum.
RXTE observations during this outburst indicated a pulse period of 160.4 s and a cyclotron resonance scattering feature in the spectrum at ∼32 keV.
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Each feature in the spectra is labelled with the associated Pr3+ energy level transition.
The broad band at ~615 625 cm−1 is the major feature in the spectra of the samples for both groups annealed at T c ≤ 800 °C (Fig. 1a, b).
As an important feature in the spectra of ZnPCSulf with Au-SiO2, multiple Au-S stretching modes were observed at about 250 cm−1 (black spectra in Figs. 8b).
This region is approximately 75 nm thick in S100 compared to <10 nm in S25, thus the dominance of the feature in the spectra of S100 may correspond to the increased region thickness.
2Note that the 8.5μm feature in the spectra of NGC 7023 and IRAS 01005+7910 is essentially invisible because of severe blending with the AIB at 8.6μm, and the 7.0 μm feature in Tc1 is contaminated with a [Ar II] line at 7.0μm.
Not surprisingly, many users eventually run their spectrometers minimally sampled, and then find that they need yet more resolution to resolve the features in the spectrum.
The HSP is to synthesize the fault related features in the spectrum, whereas LSA is to extract fault indicators for incipient IM air-gap eccentricity fault detection.
"Negative" structural constraints, which are introduced because of the absence of some characteristic features in the spectrum, are commonly more informative than positive constraints.
Besides rotation, another factor that can widen the absorption features in the spectrum of a star is pressure broadening.
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