[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-6361&DestApp=JCR&RQ=IF_CAT_BOXPLO
Iron, the universe’s most abundant refractory element, is highly depleted in both circumstellar and ...
International audienceWe investigate the relationship between the dust-to-metals ratio (D/M) and the...
Context: The Cepheid period-luminosity (PL) relation is unquestionably one of the most powerful tool...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of ...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of O...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of O...
We present a fit to the spectral energy distribution of OH 127.8+0.0, a typical asymptotic giant bra...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
The mineralogy of the dense, dusty superwind of OH/IR stars can provide important constraints for un...
We examine the mid-infrared fluxes and spectral energy distributions for stars with iron abundances ...
We examine the mid-infrared fluxes and spectral energy distributions for stars with iron abundances ...
We present a systematic study of the effect of metallicity on the stellar spectral energy distributi...
Abstract only availableCircumstellar dust is the key to understanding the cosmos. Circumstellar dust...
Title 2.4-197 micron spectroscopy of OH/IR stars: the IR characteristics of circumstellar dust in O-...
Context. Most studies devoted to Herbig Ae/Be stars (HAeBes) assume solar metallicity. However, the ...
Iron, the universe’s most abundant refractory element, is highly depleted in both circumstellar and ...
International audienceWe investigate the relationship between the dust-to-metals ratio (D/M) and the...
Context: The Cepheid period-luminosity (PL) relation is unquestionably one of the most powerful tool...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of ...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of O...
Submitted to: Astron. Astrophys. Abstract: We present a fit to the spectral energy distribution of O...
We present a fit to the spectral energy distribution of OH 127.8+0.0, a typical asymptotic giant bra...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
The mineralogy of the dense, dusty superwind of OH/IR stars can provide important constraints for un...
We examine the mid-infrared fluxes and spectral energy distributions for stars with iron abundances ...
We examine the mid-infrared fluxes and spectral energy distributions for stars with iron abundances ...
We present a systematic study of the effect of metallicity on the stellar spectral energy distributi...
Abstract only availableCircumstellar dust is the key to understanding the cosmos. Circumstellar dust...
Title 2.4-197 micron spectroscopy of OH/IR stars: the IR characteristics of circumstellar dust in O-...
Context. Most studies devoted to Herbig Ae/Be stars (HAeBes) assume solar metallicity. However, the ...
Iron, the universe’s most abundant refractory element, is highly depleted in both circumstellar and ...
International audienceWe investigate the relationship between the dust-to-metals ratio (D/M) and the...
Context: The Cepheid period-luminosity (PL) relation is unquestionably one of the most powerful tool...