High S/N echelle data of chi Lupi have been obtained at 36 different wavelength settings. The high resolution of the observations combined with the low rotational velocity of chi Lupi (v sin i approximate to 1 km s(-1)), allow the UV spectrum of this star to be seen with unprecedented detail, and provides a unique resource for the study of both atomic physics and stellar atmospheres
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of planetary f...
Observations of the ultra-sharp-lined, chemically peculiar star chi Lupi taken by the Goddard High R...
The HST has provided visual images of the universe of unprecedented clarity and sensitivity. It is l...
We summarize here the results of a major eight-year investigation of the extraordinarily detailed UV...
Observations of the ultra-sharp-lined HgMn star chi Lupi made with the Goddard High Resolution Spect...
Eta Carinae is a super-massive, super-luminous star. It is surrounded by a bipolar nebula, the "Homu...
This paper presents the first study of the properties of the peculiar emission-line star GG Carinae ...
We report on experimental absolute oscillator strengths for 18 UV lines of Ru II, obtained by combin...
The determination of elemental abundances plays an important role inunderstanding the atmospheric pr...
Abundances for the elements W, Os, and Bi are presented for the HgMn star chi Lupi, based upon GHRS ...
The near-infrared spectrum of upsilon Sagittarii has been registered using the SOFIN high resolution...
The mass accretion rate is a crucial parameter for the study of the evolution of accretion discs aro...
We present an Atlas of the high resolution spectrum of the VV Cep M1-2Iab + Be variable KQ Pup (Boss...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of planetary f...
Observations of the ultra-sharp-lined, chemically peculiar star chi Lupi taken by the Goddard High R...
The HST has provided visual images of the universe of unprecedented clarity and sensitivity. It is l...
We summarize here the results of a major eight-year investigation of the extraordinarily detailed UV...
Observations of the ultra-sharp-lined HgMn star chi Lupi made with the Goddard High Resolution Spect...
Eta Carinae is a super-massive, super-luminous star. It is surrounded by a bipolar nebula, the "Homu...
This paper presents the first study of the properties of the peculiar emission-line star GG Carinae ...
We report on experimental absolute oscillator strengths for 18 UV lines of Ru II, obtained by combin...
The determination of elemental abundances plays an important role inunderstanding the atmospheric pr...
Abundances for the elements W, Os, and Bi are presented for the HgMn star chi Lupi, based upon GHRS ...
The near-infrared spectrum of upsilon Sagittarii has been registered using the SOFIN high resolution...
The mass accretion rate is a crucial parameter for the study of the evolution of accretion discs aro...
We present an Atlas of the high resolution spectrum of the VV Cep M1-2Iab + Be variable KQ Pup (Boss...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Aims. A set of new, sensitive, and spectrally resolved, sub-millimeter line observations are used to...
Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of planetary f...