PhDAstronomyAstrophysicsUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://deepblue.lib.umich.edu/bitstream/2027.42/184933/2/6717764.pd
International audienceFaint high-latitude carbon stars (FHLCs) are distant, luminous giants. For thi...
In a previous paper, we assembled a collection of medium-resolution spectra of 35 carbon stars, cove...
PhDAstronomyAstrophysicsUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://d...
We have developed a classiÐcation system for the infrared spectral emission from carbon stars, using...
Carbon stars are relatively uncommon, luminous, cool stars whose spectra exhibit exceptionally stron...
ABSTRACT. We have identified 139 cool carbon stars in the near-infrared spectrophotometric survey of...
We analysed the spectral energy distribution of the evolved carbon star DY Per by spectral synthesis...
We have searched for the 3.1 mum absorption feature, a well-known characteristic of optical carbon s...
[[sponsorship]]天文及天文物理研究所[[note]]出版中(submitted);[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge....
This report gives an update of developments (since the last General Assembly at Prague) in the areas...
A catalogue of 7760 carbon stars in the Large Magellenic Cloud is presented. The stars were identif...
Context. Stars evolving along the asymptotic giant branch (AGB) can become carbon rich in the final ...
We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-Shooter instru...
International audienceThis study is about carbon stars detected in a program of spectral type determ...
We have identified 139 cool carbon stars in the near-infrared spectro-photometric survey of the Infr...
International audienceFaint high-latitude carbon stars (FHLCs) are distant, luminous giants. For thi...
In a previous paper, we assembled a collection of medium-resolution spectra of 35 carbon stars, cove...
PhDAstronomyAstrophysicsUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://d...
We have developed a classiÐcation system for the infrared spectral emission from carbon stars, using...
Carbon stars are relatively uncommon, luminous, cool stars whose spectra exhibit exceptionally stron...
ABSTRACT. We have identified 139 cool carbon stars in the near-infrared spectrophotometric survey of...
We analysed the spectral energy distribution of the evolved carbon star DY Per by spectral synthesis...
We have searched for the 3.1 mum absorption feature, a well-known characteristic of optical carbon s...
[[sponsorship]]天文及天文物理研究所[[note]]出版中(submitted);[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge....
This report gives an update of developments (since the last General Assembly at Prague) in the areas...
A catalogue of 7760 carbon stars in the Large Magellenic Cloud is presented. The stars were identif...
Context. Stars evolving along the asymptotic giant branch (AGB) can become carbon rich in the final ...
We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-Shooter instru...
International audienceThis study is about carbon stars detected in a program of spectral type determ...
We have identified 139 cool carbon stars in the near-infrared spectro-photometric survey of the Infr...
International audienceFaint high-latitude carbon stars (FHLCs) are distant, luminous giants. For thi...
In a previous paper, we assembled a collection of medium-resolution spectra of 35 carbon stars, cove...
PhDAstronomyAstrophysicsUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttp://d...