The ratio of neutral hydrogen to neutral helium in the local interstellar medium
The results are described from a sounding rocket borne EUV spectrometer that was designed and built. This instrument operated from 400 to 1150A with a spectral resolution of approx. 15A. The instrument effective area was about 1 sq cm. The instrument was successfully launched, and observed the nearby DA white dwarf G191-B2B. From this observation, it was determined that the stellar effective temperature is 61,000 + or -4000 to 6000K, and the ratio of helium to hydrogen in the stellar photosphere is 1.0 + or -0.68 to 2.2 x 10(exp -4). Additionally, the neutral column densities of helium and hydrogen were measured to the star. The neutral helium column density was determined from the first observation of the interstellar absorption edge at 504A. The ratio of neutral helium to neutral hydrogen constrains the mean ionization of the warm gas along the line of sight to G191-B2B. The fractional ionization of hydrogen (H II/H) is approx. less than 20 percent, unless significant helium ionization is present as well. The scenario where the fractional ionization of hydrogen is high (H II/H) approx. less than 40 percent and the helium is neutral is ruled out with 99 percent certainty. This result is consistent with some recent theoretical calculations. Using these results, a self-consistent model of the local interstellar medium along the line of sight to G191-B2B is developed. In addition, an unexpected emission feature at 584A was detected in this observation with a high level of significance. Possible sources of this emission are examined, including the companion K dwarf G191-B2A, and an emission nebula near or around G191-B2B.
- Research Organization:
- California Univ., Berkeley, CA (USA)
- OSTI ID:
- 6690299
- Country of Publication:
- United States
- Language:
- English
Similar Records
Rocket and satellite observations of the local interstellar medium
Possible detection of an emission feature near 584 A in the direction of G191-B2B
Related Subjects
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
DATA
ELECTROMAGNETIC RADIATION
ELEMENTS
EMISSION SPECTRA
EXPERIMENTAL DATA
EXTREME ULTRAVIOLET RADIATION
FLUIDS
GASES
HELIUM
HYDROGEN
INFORMATION
INTERSTELLAR SPACE
NEBULAE
NONMETALS
NUMERICAL DATA
PHOTOSPHERE
RADIATIONS
RARE GASES
SOLAR ATMOSPHERE
SPACE
SPECTRA
ULTRAVIOLET RADIATION