We carried out a detailed analysis of the helium lines at 4921, 5876 and 6678 A in the spectra of the HgMn stars HD 58661, HD 172044, HD 185330 and HD 186122. For the first of these lines, the isotopic shift reaches +0.33 A for pure 3He, while for the last one, the maximum shift is +0.50 A. The 5876 line does not show any significant isotopic shift and is chosen for comparison. No trace of 3He was found in the atmosphere of HD 172044, while its presence was confirmed in HD 185330. This isotope is clearly present in the atmosphere of HD 58661. The results obtained for HD 186122 were ambiguous, 3He being apparently present in the 4921 line but not in the 6678 line, possibly because the latter is very weak
We recall the current status of the long-standing 3He problem, and its possible connection with chem...
We follow the evolution of "3He in stars of mass 0.8... 10M_sun for Pop. I and II compositions ...
International audienceThe light isotope of helium, 3He, is essentially a primordial substance entrap...
We have used the CFHT and Gemini South telescopes to obtain high-resolution, high signal-to-noise op...
Decades ago, 3He isotope enrichment in helium-weak B-type main-sequence, in blue horizontal branch a...
We follow the evolution of 3He in stars of mass 0.8 -- 10 M (solar units) for Pop. I and II composit...
Several B-type main-sequence stars show chemical peculiarities. A particularly striking class are th...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
Cosmic ray ^3He/^4He observations, including a new measurement at ~65 MeV/nucleon from ISEE-3, are c...
The rare isotopes H-2 and He-3 in cosmic rays are believed to be of secondary origin produced by nuc...
The isotopes ^2H and ^3He have been identified in low-energy cosmic rays during solar-quiet periods ...
The purpose of this work is to refine our knowledge about the nature of helium with a high abundance...
Atmospheric parameters and helium abundances of 44 bright subdwarf B stars have been determined. Mor...
Recent observations by Bania et al. (2002) measure He3 versus oxygen in Galactic HII regions, findin...
To understand the chemical evolution of the Galaxy, we need to understand the contribution of PNe in...
We recall the current status of the long-standing 3He problem, and its possible connection with chem...
We follow the evolution of "3He in stars of mass 0.8... 10M_sun for Pop. I and II compositions ...
International audienceThe light isotope of helium, 3He, is essentially a primordial substance entrap...
We have used the CFHT and Gemini South telescopes to obtain high-resolution, high signal-to-noise op...
Decades ago, 3He isotope enrichment in helium-weak B-type main-sequence, in blue horizontal branch a...
We follow the evolution of 3He in stars of mass 0.8 -- 10 M (solar units) for Pop. I and II composit...
Several B-type main-sequence stars show chemical peculiarities. A particularly striking class are th...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
Cosmic ray ^3He/^4He observations, including a new measurement at ~65 MeV/nucleon from ISEE-3, are c...
The rare isotopes H-2 and He-3 in cosmic rays are believed to be of secondary origin produced by nuc...
The isotopes ^2H and ^3He have been identified in low-energy cosmic rays during solar-quiet periods ...
The purpose of this work is to refine our knowledge about the nature of helium with a high abundance...
Atmospheric parameters and helium abundances of 44 bright subdwarf B stars have been determined. Mor...
Recent observations by Bania et al. (2002) measure He3 versus oxygen in Galactic HII regions, findin...
To understand the chemical evolution of the Galaxy, we need to understand the contribution of PNe in...
We recall the current status of the long-standing 3He problem, and its possible connection with chem...
We follow the evolution of "3He in stars of mass 0.8... 10M_sun for Pop. I and II compositions ...
International audienceThe light isotope of helium, 3He, is essentially a primordial substance entrap...