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The Stellar Structure of Irregular Galaxies. Face-on Galaxies
DOI: 10.1134/1.1985947 Bibcode: 2005ARep...49..501T

Tikhonov, N. A.

Stellar photometry of nearby irregular galaxies of the Local Group is used to identify and study the young and old stellar populations of these galaxies. An analysis of the spatial distributions of stars of different ages in face-on galaxies shows that the young stellar populations in irregular galaxies are concentrated toward the center, and form…

2005 Astronomy Reports
eHST 22
Turbulence in the Inner Solar Wind Determined from Frequency Fluctuations of the Downlink Signals from the ULYSSES and GALILEO Spacecraft
DOI: 10.1134/1.1941491 Bibcode: 2005ARep...49..485E

Plettemeier, D.; Bird, M. K.; Efimov, A. I. +2 more

The results of several sets of measurements of the frequency of radio signals during coronal-sounding experiments carried out from 1991 to 2000 using the ULYSSES and GALILEO spacecraft are presented and analyzed. The S-band signals (carrier frequency f = 2295 MHz) were received at the three 70-m widely spaced ground stations of the NASA Deep Space…

2005 Astronomy Reports
Ulysses 15
Large-scale activity in solar eruptive events of October November 2003 observed from SOHO/EIT data
DOI: 10.1134/1.1862362 Bibcode: 2005ARep...49..155C

Grechnev, V. V.; Chertok, I. M.

Large-scale solar disturbances associated with powerful flares and coronal mass ejections (CMEs) during two passages of a grand system of three active regions in October November 2003 are analyzed using data obtained with the SOHO/EIT EUV telescope. Dimmings (transient coronal holes) and, to a lesser extent, coronal waves (traveling emitting front…

2005 Astronomy Reports
SOHO 13
A Spectroscopic and Photometric Study of NGC 2685, the Prototype Polar-Ring Galaxy
DOI: 10.1134/1.2139811 Bibcode: 2005ARep...49..958H

Moiseev, A. V.; Burenkov, A. N.; Hagen-Thorn, V. A. +3 more

We present and analyze spectroscopic and photometric observations for NGC 2685, the prototype polar-ring galaxy. The spectroscopic data were acquired using the 6 m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences with the UAGS spectrograph and a scanning Fabry-Perot interferometer, while the photometric analysi…

2005 Astronomy Reports
eHST 6