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Linear Spectropolarimetry of Young and Other Emission Line Stars
The aim of this article is to demonstrate the useful role that can be played by spectropolarimetric observations of young and evolved emission line... -
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Iron Line Emission in X-Ray Afterglows
Recent observations of X-ray afterglows reveal the presence of a redshifted K... -
4.7 μm CO and H2 Line Emission in NGC 2071
Two lines of the fundamental vibration-rotation band of carbon monoxide at 4.7 μm have been detected in emission in the NGC 2071 IR out.ow region,... -
Modeling Emission Line Galaxies
Predicting the emission line signals from galaxies and IGM observed in the future experiments is crucial for their interpretation as well as for... -
Analysis of Emission Line Widths of [CII] 158μm
A study of [CII] 158 μm emission line profiles observed with Herschel PACS for 379 galaxies is presented. Emission line widths are compared to [CII]...
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Hi line analysis of Herbig Ae/Be stars using X-Shooter spectra
Herbig Ae/Be stars are intermediate-mass pre-main sequence stars undergoing accretion through their circumstellar disk. The optical and infrared (IR)...
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Isolated Neutron Stars
Non-accreting neutron stars display diverse characteristics, leading us to classify them into several groups. This chapter is an observational driven... -
Isolated Neutron Stars
Non-accreting neutron stars display diverse characteristics, leading us to classify them into several groups. This chapter is an observational driven... -
Formation of Stars
In this chapter we discuss the formation of stars. The formation of stars can be observed in various gas nebulae, and the formation process is... -
Herbig Stars
Herbig Ae/Be stars are young contracting stars on the radiative track in the HR diagram on their way to the main sequence. These stars provide a...
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VLT/ISAAC Spectroscopy of Young Massive Stars Embedded in Ultra-Compact H II Regions
Using ISAAC mounted at the Very Large Telescope, we have obtained medium-resolution K-band spectra of newly formed massive stars, which are deeply... -
Metallicity of Young Stars of the NGC 4068 Galaxy
AbstractBased on archival images from the Hubble Space Telescope, stellar photometry of the galaxy NGC 4068 was carried out. The resulting...
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Fundamental Physics with Neutron Stars
Neutron stars are rich laboratories of multiple branches of modern physics. These include gravitational physics, nuclear and particle physics,... -
Chains of mini-boson stars
In this paper, we re-investigate the static, soliton-like solutions in the model of the Einstein gravity coupled to a free and complex scalar field,...
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Estimation of stellar parameters and mass accretion rate of classical T Tauri stars from LAMOST DR6
Classical T Tauri stars (TTS) are low-mass pre-main sequence stars with an active circumstellar environment. In this work, we present the...
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Magnetic Field Structures of Chemically Peculiar Stars. I. HD57682, HD81009
Based on published data on the magnitudes of the magnetic field, models of the magnetic field of magnetic stars of various types of peculiarity...
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Periodicity of Flare Frequency of Active Flare Stars Detected by Tess
Data from the TESS orbital observatory are used to study the most active flare stars indicating 100 or more flares during the period from July 2018...
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The Digitized First Byurakan Survey Data Base. Late-Type Stars Candidates. New Confirmations. I
The Digitized First Byurakan Survey (DFBS) is the digitized version of the First Byurakan Survey (FBS, or Markarian survey). The FBS was the first...