Add to ORKGThe spectral distribution of pairs of stars within the same spectral type and luminosity class, one of which is reddened and the other unreddened is compared. It is assumed that the observed difference between two stars is only attributed to the interstellar medium. Their physical properties, size distribution of particles, geometrical shape, and their location in space are considered
Deriving the physical properties of red supergiants (RSGs) depends on accurate corrections for redde...
The dust reddening law from the UV to the near-IR for the extended regions of galaxies is here deriv...
Extended Red Emission (ERE) has been detected in many dusty astrophysical objects and this raises th...
Filter photometry has been used to derive the interstellar reddening law from stars through the stud...
Objective prism spectra obtained with the 16/24/60-inch Schmidt telescope have been used for an inv...
The mystery of Canis Major overdensity is addressed. We discuss concurrent methods and their limitat...
This paper examines the relationship between spectra of stars of same spectral type with extremely l...
The wavelength dependence of interstellar obscuration, in magnitudes against reciprocal wavelength,...
The interstellar reddening law is investigated along the Galactic equator near the Cam, Per and Cas ...
We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digita...
Some of the diffuse interstellar features (DIBs) in the spectra of certain stars at high galactic la...
New spectral types and photometry are reported for numerous stars in Sco OB-1 and in the foreground ...
International audienceDeriving the physical properties of red supergiants (RSGs) depends on accurate...
The band-width effect on interstellar reddening lines in the J-H vs. H-Ks diagram of the 2MASS surve...
This thesis presents an investigation into the reddening effects of the diffuse ISM using a subset o...
Deriving the physical properties of red supergiants (RSGs) depends on accurate corrections for redde...
The dust reddening law from the UV to the near-IR for the extended regions of galaxies is here deriv...
Extended Red Emission (ERE) has been detected in many dusty astrophysical objects and this raises th...
Filter photometry has been used to derive the interstellar reddening law from stars through the stud...
Objective prism spectra obtained with the 16/24/60-inch Schmidt telescope have been used for an inv...
The mystery of Canis Major overdensity is addressed. We discuss concurrent methods and their limitat...
This paper examines the relationship between spectra of stars of same spectral type with extremely l...
The wavelength dependence of interstellar obscuration, in magnitudes against reciprocal wavelength,...
The interstellar reddening law is investigated along the Galactic equator near the Cam, Per and Cas ...
We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digita...
Some of the diffuse interstellar features (DIBs) in the spectra of certain stars at high galactic la...
New spectral types and photometry are reported for numerous stars in Sco OB-1 and in the foreground ...
International audienceDeriving the physical properties of red supergiants (RSGs) depends on accurate...
The band-width effect on interstellar reddening lines in the J-H vs. H-Ks diagram of the 2MASS surve...
This thesis presents an investigation into the reddening effects of the diffuse ISM using a subset o...
Deriving the physical properties of red supergiants (RSGs) depends on accurate corrections for redde...
The dust reddening law from the UV to the near-IR for the extended regions of galaxies is here deriv...
Extended Red Emission (ERE) has been detected in many dusty astrophysical objects and this raises th...