WebApr 22, 2024 · By definition, classical Be stars are hot, non-supergiant, non-radially pulsating, rapidly rotating B-type stars, which show or have shown one or more Balmer lines in emission (most prominently in H α) [24,25,26]. Their rotation speeds are presumed to be near their critical velocity and they have strong stellar winds and a high mass-loss rate. WebIt is concluded that the present data do not justify the attribution of the short-lived optical emission to the presumed hard X-ray producing electrons. We evaluate the possibility that …
Hydrogen and Deuterium Spectroscopy - School of Physics …
WebWe present further results of the optical observations of the 3C 390.3 nucleus undertaken at the Crimean Astrophysical Observatory since 1992. From the new data obtained in 2000–2007, we find... Balmer lines can appear as absorption or emission lines in a spectrum, depending on the nature of the object observed. In stars, the Balmer lines are usually seen in absorption, and they are "strongest" in stars with a surface temperature of about 10,000 kelvins (spectral type A). See more The Balmer series, or Balmer lines in atomic physics, is one of a set of six named series describing the spectral line emissions of the hydrogen atom. The Balmer series is calculated using the Balmer formula, an See more Balmer noticed that a single wavelength had a relation to every line in the hydrogen spectrum that was in the visible light region. That … See more • Astronomical spectroscopy • Bohr model • Hydrogen spectral series • Lyman series • Rydberg formula See more The Balmer series is characterized by the electron transitioning from n ≥ 3 to n = 2, where n refers to the radial quantum number or principal quantum number of the electron. The … See more The Balmer series is particularly useful in astronomy because the Balmer lines appear in numerous stellar objects due to the abundance of hydrogen in the universe, and therefore are commonly seen and relatively strong compared to lines from other elements. See more film prince of foxes
Optical spectroscopy of Be stars: peak separation of …
WebSep 1, 2003 · Quasars with intrinsically red (optically steep) power-law continua tend to have narrower Balmer lines and weaker C IV, C III], He II, and 3000 Å bump emission as … WebMar 1, 2002 · An optical emission spectroscopy (OES) method was employed for diagnostic analysis of the plasma during the processes. In this study, AISI H13 steels were nitrided at 550 °C for 4 h with various discharge times and nitrogen concentrations. ... especially those involved directly in the surface treatment processes, ... Also, Balmer line H ... grover\u0027s pay and pack nampa