Publications by authors named "V G Doroshenko"

Gliomas are a group of primary brain tumors characterized by their aggressive nature and resistance to treatment. Infiltration of surrounding normal tissues limits surgical approaches, wide inter- and intratumor heterogeneity hinders the development of universal therapeutics, and the presence of the blood-brain barrier reduces the efficiency of their delivery. As a result, patients diagnosed with gliomas often face a poor prognosis and low survival rates.

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SS 433 is a microquasar, a stellar binary system that launches collimated relativistic jets. We observed SS 433 in gamma rays using the High Energy Stereoscopic System (H.E.

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Article Synopsis
  • The Milky Way's center contains a dormant black hole, Sagittarius A (Sgr A), with a mass of about 4 million solar masses and low luminosity compared to active galactic nuclei.
  • Researchers have studied X-ray reflections from surrounding dense gas to investigate Sgr A's past activity, suggesting it flared up significantly in the past.
  • Observations from the Imaging X-ray Polarimetry Explorer revealed a 31% polarization degree in X-rays, indicating Sgr A was much more active around 200 years ago, with luminosity similar to that of a Seyfert galaxy.
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Corynebacterium glutamicum AJ1511 and Escherichia coli BW25113 strains were compared in terms of resistance to sarcosine (N-methylglycine). The E. coli strain was more sensitive to sarcosine than C.

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Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years) and located inside an extended structure called Vela X, which is itself inside the supernova remnant. Previous X-ray observations revealed two prominent arcs that are bisected by a jet and counter jet.

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