Search Publications

Apex diagrams for the stellar population of the solar neighborhood
DOI: 10.1134/S1063772909030068 Bibcode: 2009ARep...53..243V

Vereshchagin, S. V.; Reva, V. G.; Chupina, N. V.

We have studied some kinematic features of the coronas of near-solar stellar streams, based on Hipparcos observations. Apex diagrams for kinematic streams, open clusters, and field stars are plotted. In our analysis, we used the apex-diagram (AD) method we developed earlier. We find that the Eggen streams and Arcturus stream have similar propertie…

2009 Astronomy Reports
Hipparcos 1
Flare Loop Sizes in Young Suns
Bibcode: 2009BaltA..18..233V

Schultz, J.; Nevalainen, J.; Väänänen, M. K.

We analyse 27 solar flares observed with GOES and RHESSI in the X-ray bands at 3.1--24.8 keV and 12--25 keV and in Hα . The flaring region diameter in X-rays is found to correlate with the Hα decay duration, and this correlation is used to approximate the flare loop semilength. We propose the method to measure the coronal loop semilengths in young…

2009 Baltic Astronomy
XMM-Newton 1
Structural Analysis of A2034 Clusters of Galaxies
Bibcode: 2009POBeo..86..301B

Hudaverdi, M.; Ercan, E. N.; Bozkurt, M.

We present the analysis of X-ray and optical observations of Abell 2034. It is located at the moderate redshift of z=0.113. X-ray data are taken from the XMM-Newton archive. The best-fit single temperature of 7.6 keV model well defines the diffuse hot plasma. The cluster is observed by ground based optical Turkish National Observatory RTT-150 tele…

2009 Publications de l'Observatoire Astronomique de Beograd
XMM-Newton 1
Coronal dynamics and heating theories
DOI: 10.1016/j.asr.2008.05.012 Bibcode: 2009AdSpR..43..108G

Gudiksen, Boris V.

A large number of coronal heating theories have been proposed and most of them can be labeled as AC or DC heating theories. Here a short description of these two main theories is given, and the results of a DC heating model simulation is explained in more detail. As a result of that model, arguments are given for putting emphasis on launching a ve…

2009 Advances in Space Research
SOHO 1
Polycyclic aromatic hydrocarbon selected galaxies
DOI: 10.1051/0004-6361/200912705 Bibcode: 2009A&A...507..713H

Siebenmorgen, R.; Haas, M.; Chini, R. +3 more

Context: This is the fourth in a series of papers based on the ISOCAM Parallel Survey at 6.7 µm. While the first three papers have been devoted to active galactic nuclei (AGN), here we report on emission-line galaxies without AGN signatures in their optical spectra.
Aims: Polycyclic aromatic hydrocarbon (PAH) emission has been found in b…

2009 Astronomy and Astrophysics
ISO 1
Revealing Probable Universal Features in the Lower Red Giant Branch Luminosity Functions of Galactic Globular Clusters
DOI: 10.1088/0004-6256/137/6/5110 Bibcode: 2009AJ....137.5110K

Kravtsov, V. V.

This paper aims at demonstrating, for the first time, very probable universal peculiarities of the evolution of stars in the lower red giant branch (RGB) of Galactic globular clusters (GCs), reflected in two corresponding dips in the luminosity functions (LFs). By relying on the database of Hubble Space Telescope photometry of GCs, we analyze the …

2009 The Astronomical Journal
eHST 1
X-Ray Analysis of Galactic SNR G27.4+0.0
Bibcode: 2009POBeo..86...89S

Hudaverdi, M.; Ercan, E. N.; Sezer, A. +2 more

In this work, we present X-ray analysis result of SNR G27.4+0.0 observed by XMM-Newton satellite. Three EPIC detectors are studied comparatively. The spatial and spectral analysis are performed, 0.3-10 keV (all band). In order to define possible distribution of interested abundances soft, medium and hard X-ray images are constructed. NEI (Non-equi…

2009 Publications de l'Observatoire Astronomique de Beograd
XMM-Newton 1
GRB observed by IBIS/PICsIT in the MeV energy range
DOI: 10.1016/j.asr.2009.01.002 Bibcode: 2009AdSpR..43.1055B

Götz, D.; Foschini, L.; Di Cocco, G. +5 more

We present the preliminary results of a systematic search for GRB and other transients in the publicly available data for the IBIS/PICsIT (0.2-10 MeV) detector on board INTEGRAL. Lightcurves in 2-8 energy bands with time resolution from 1 to 62.5 ms have been collected and an analysis of spectral and temporal characteristics has been performed. Th…

2009 Advances in Space Research
INTEGRAL 1
Hard X-ray flux from low-mass stars in the Cygnus OB2 association
DOI: 10.1051/0004-6361/200811342 Bibcode: 2009A&A...503..505C

Micela, G.; Drake, J. J.; Flaccomio, E. +1 more

Context: The Cygnus OB2 association, the central engine of the Cygnus X star-forming region, is the subject of an extensive INTEGRAL Key Project that will accumulate 6Ms of observations. Analysis of 2Ms of observations by De Becker and co-workers provides the most sensitive limit yet obtained on hard X-ray emission from the cluster.
Aims: We i…

2009 Astronomy and Astrophysics
INTEGRAL 1
Streaming Circumnuclear Gas of the Seyfert 2 Galaxy NGC 5728
DOI: 10.5303/JKAS.2009.42.5.125 Bibcode: 2009JKAS...42..125S

Ferruit, Pierre; Hyung, Siek; Son, Dong-Hoon +1 more

2009 Journal of Korean Astronomical Society
IUE 1