Identify physical conditions of B-emission stars at certain positions over specific wavelengths. Classify stars based on colors and Identify the spectral type of a star and temperature based on its absorption lines. Summarize the changes and excess in flux over certain wavelengths of multiple B-emission stars while also looking at the flux when filtered over the V, B, U and K bands. Identify properties of the Be stars and evaluate how changing certain properties effect the stars and their surrounding disks
Massive O- and B-type stars are cosmic engines in the Universe and can be the dominant source of l...
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, com...
Emission-line stars in young open clusters are identified to study their properties, as a function o...
We present spectrophotometric data from 0.4 μm to 4.2 μm for bright, northern sky, Be stars and seve...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Be stars are rapidly rotating B-type stars that possess a gaseous disk formed by matter released fro...
We describe the behaviour of IR hydrogen emission lines of a sample of Be stars and discuss the phys...
We describe the behaviour of IR hydrogen emission lines of a sample of Be stars and discuss the phys...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
Context. A recent analysis of visual Fell emission lines of 17 classic Be stars using the self-absor...
We present H band (1.53 - 1.69 micron) spectra of 57 isolated Be stars of spectral types O9-B9 and l...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present a spectroscopic study of 150 Classical Be stars in 39 open clusters using medium resoluti...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
Massive O- and B-type stars are cosmic engines in the Universe and can be the dominant source of l...
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, com...
Emission-line stars in young open clusters are identified to study their properties, as a function o...
We present spectrophotometric data from 0.4 μm to 4.2 μm for bright, northern sky, Be stars and seve...
We present infra-red (JHK) photometry of 52 isolated Be stars of spectral types O9-B9 and luminosity...
Be stars are rapidly rotating B-type stars that possess a gaseous disk formed by matter released fro...
We describe the behaviour of IR hydrogen emission lines of a sample of Be stars and discuss the phys...
We describe the behaviour of IR hydrogen emission lines of a sample of Be stars and discuss the phys...
AcceptedInternational audienceContext. Classical Be stars are hot non-supergiant stars surrounded by...
AbstractWe present theoretical infrared images for Be star disks as projected on the plane of the sk...
Context. A recent analysis of visual Fell emission lines of 17 classic Be stars using the self-absor...
We present H band (1.53 - 1.69 micron) spectra of 57 isolated Be stars of spectral types O9-B9 and l...
Context. Be stars are fast-rotating early-type emission line stars. It is generally assumed that obs...
We present a spectroscopic study of 150 Classical Be stars in 39 open clusters using medium resoluti...
Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still und...
Massive O- and B-type stars are cosmic engines in the Universe and can be the dominant source of l...
Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, com...
Emission-line stars in young open clusters are identified to study their properties, as a function o...