Show/Hide Menu
Hide/Show Apps
Logout
Türkçe
Türkçe
Search
Search
Login
Login
OpenMETU
OpenMETU
About
About
Open Science Policy
Open Science Policy
Open Access Guideline
Open Access Guideline
Postgraduate Thesis Guideline
Postgraduate Thesis Guideline
Communities & Collections
Communities & Collections
Help
Help
Frequently Asked Questions
Frequently Asked Questions
Guides
Guides
Thesis submission
Thesis submission
MS without thesis term project submission
MS without thesis term project submission
Publication submission with DOI
Publication submission with DOI
Publication submission
Publication submission
Supporting Information
Supporting Information
General Information
General Information
Copyright, Embargo and License
Copyright, Embargo and License
Contact us
Contact us
Optical search for Supernova Remnants in two-spiral galaxies
Date
2005-09-30
Author
Akyüz, Ahmet Oğuz
Bhattacharya, D
Sonbas, E
Cekmecelioglu, E
Metadata
Show full item record
This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
.
Item Usage Stats
77
views
0
downloads
Cite This
We present the results of an optical search for Supemova Remnants (SNRs) in the spiral galaxies NGC6946 and NGC628. The SNR identification technique consisted of constructing continuum-subtracted H-alpha and [SII] lambda lambda 6716,6731 images and then using [SII] / H-alpha ratios obtained from the image. 32 emission nebulae have been detected as SNR candidates in NGC6946. 22 of them were previously identified by Matonick et al (1997). We found five SNR candidates in the spiral galaxy NGC628. We will compare and contrast the new SNR candidates and our optical data with the existing Chandra and XMM observation of the two galaxies of interest and VLA radio observation of NGC6946. Interference-filter CCD images of two spiral galaxies were taken in 2004 September with the f/7.7 1.5 m Russian-Turkish Telescope at Turkish National Observatory.
Subject Keywords
SNR
,
Optical observation
URI
https://hdl.handle.net/11511/53919
Collections
Department of Computer Engineering, Conference / Seminar
Suggestions
OpenMETU
Core
Efficient and accurate electromagnetic analysis of three-dimensional nano-optical structures
Yazar, Şirin; Sür, Cem Gürkan; Solak, Birol; Eroğlu, Ömer; Altınoklu, Aşkın; Güler, Sadri; Gür, Uğur Meriç; Karaosmanoğlu, Barışcan; Ergül, Özgür Salih (2017-07-08)
We present computational analysis of optical nanostructures, including but not limited to frequency-selective surfaces, metamaterials, nanoantennas, nanowires, and photonic crystals. A rigorous implementation based on surface integral equations and the multilevel fast multipole algorithm is developed for the analysis of such three-dimensional complex structures, without resorting to infinity, self-similarity, periodicity or homogeneity assumptions. The developed simulation environment provides accurate anal...
Electronic structure of a many-electron spherical quantum dot with an impurity
Sahin, M; Tomak, Mehmet (American Physical Society (APS), 2005-09-01)
We investigate the electronic structure of a many-electron spherical quantum dot with and without hydrogenic impurity. The number of electrons is taken as N=18. The density functional theory is used within local density approximation. Total energy, chemical potential, addition energy spectra, and the shell structure are determined and the results obtained are compared for cases with and without impurity. It is observed that the capacitive energy with the impurity increases in the 1s shell with respect to th...
STRUCTURAL ANALYSIS OF A2034 CLUSTERS OF GALAXIES
Bozkurt, M.; Hudaverdi, M.; ERCAN, ENİSE NİHAL (2008-10-05)
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 telescope. X-ray spectra of the individual sources from the cluster outskirts are studied. The intra cluster medium (ICM) temperature and metal distributions are const...
BINARY CLUSTERS OBSERVED WITH XMM-NEWTON X-RAY OBSERVATORY
Beygu, B.; Hudaverdi, M.; Ercan, N. (2008-10-05)
Clusters of galaxies are thought to form by accretion of galaxies along the cosmic filaments, and merging of clusters formed earlier. Observations and hydrodynamic simulations show the strong effects of mergers on physical conditions of the Intra Cluster Medium (ICM). In this work, we investigate five relatively nearby Abell clusters; A3705 (z= 0.089), A2440 (z= 0.090), A2933 (z= 0.092), A3888 (z= 0.152) and A115 (z= 0.193). Temperature; and metal abundance map are created using wavelet. algorithms. Peculia...
TURKISH NATIONAL OBSERVATORY (TUG) VIEW OF CLUSTERS OF GALAXIES
Hudaverdi, M.; ERCAN, ENİSE NİHAL; Bozkurt, M.; GÖK, FATMA; Aktekin, E. (2008-10-05)
We present the results of the optical observations of clusters of galaxies trough photometric observations with RTT150 telescope. We have selected a sample of 10 nearby (z < 1.2) Abell clusters from the northern sky. Properties of the extended X-ray intra-cluster medium (ICM) are studied using Chandra and XMM-Newton archival data. Considering possible relations of X-ray and radio plasma, the extended radio halo and jets are studied. The intent of our observations is to map galaxy densities in the optical ba...
Citation Formats
IEEE
ACM
APA
CHICAGO
MLA
BibTeX
A. O. Akyüz, D. Bhattacharya, E. Sonbas, and E. Cekmecelioglu, “Optical search for Supernova Remnants in two-spiral galaxies,” 2005, vol. 604, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/53919.