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Evolution of the ISM in Elliptical Galaxiesand Black Hole Growth
The hot phase of the ISM in nearby elliptical galaxies is observed to have temperatures in the range of 10 Mio degrees. While stellar wind and... -
Pretty small low-cost bandpass filter using a single square open-loop resonator with a centered stub for WLAN/Bluetooth/ZigBee/RFID and ISM band applications
In recent years, microwave filtering technologies have known great advancement and wide employment in wireless communication systems, necessitating...
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Dust in the Diffuse ISM
The nature of the dust in the dispersed interstellar medium is determined by various observational limitations, which we summarize with special... -
Metal-Poor Halo Stars as Tracers of ISM Mixing Processes During Halo Formation
We discuss a stochastic halo formation model to compute the early chemical enrichment of the interstellar medium (ISM) of the halo. Contrary to... -
Inhomogeneity in the Local ISM and Its Relation to the Heliosphere
This paper reviews past research and new studies underway of the local interstellar environment and its changing influence on the heliosphere. The...
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Sobolev LVG Analysis of Prebiotic Molecule Formamide (NH2CHO) Found in the ISM
Using known values of rotational and centrifugal distortion constants in conjunction with electric dipole moment of NH 2 CHO, we have calculated...
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ISM Dynamics Around Black Holes in Nearby (Radio) Early-Type Galaxies with HST
The black holes (BHs) at the centers of present-day bright early-type galaxies might represent the most massive endpoints for BH growth in the... -
Neutral hydrogen filaments in interstellar media: Are they physical?
The trending term “filament” is extensively used in the interstellar medium (ISM) and the star formation community, and is believed to be one of the...
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The Hot Interstellar Medium
The interstellar medium (ISM) of galaxies very often contains a gas component that reaches the temperature of several million degrees, whose physical... -
N-graphene synthesized in astrochemical ices
In our quest for the presence of large complex molecules containing a majority of carbon in the interstellar medium (ISM), the search for graphene...
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Search and study of young infrared stellar clusters
The main aim of this paper is to study both the Interstellar Medium (ISM) and the young stellar population in the three star-forming regions, namely...
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The Polstar high resolution spectropolarimetry MIDEX mission
The Polstar mission will provide a space-borne 60 cm spectropolarimeter operating at ultraviolet (UV) wavelengths, capturing all four Stokes...
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Interacting planetary nebulae III: verification and galactic population based on the measurements of Gaia EDR3
The phenomenon of interaction between planetary nebulae (PNe) and the interstellar medium (ISM) is one of the significant issues in the field of...
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Ultraviolet spectropolarimetry with polstar: interstellar medium science
Continuum polarization over the UV-to-microwave range is due to dichroic extinction (or emission) by asymmetric, aligned dust grains. Scattering can...
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Interstellar Absorption and Dust Scattering
The study of the interstellar medium (ISM) in the X-rays has entered a golden age with the advent of the X-ray observatories XMM-Newton and Chandra.... -
On the Fractional Version of Cosmic Ray Acceleration Nonlocality
AbstractThe commonly accepted CR transport theory is based on the diffusion equation, which in turn follows from the Boltzmann kinetic equation. The...
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On the Classical Approach to Describing the Diffusion of Cosmic Rays in a Turbulent Medium
AbstractThe inhomogeneous structure of the interstellar medium (ISM) is characterized by large-scale fluctuations that significantly affect the...