Photometric Study of the Seyfert Galaxy NGC 4151
The results of CCD photometry in the Johnson-Morgan BV R system for the Seyfert galaxy NGC 4151 are reported. The observations were carried out from November 15, 2013 to May 13, 2016 with the 1-m telescope of Tien-Shan Astronomical Observatory of the Fesenkov Astrophysical Institute. An analysis of...
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| Format: | Article |
| Language: | English |
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De Gruyter
2016-09-01
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| Series: | Open Astronomy |
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| Online Access: | https://doi.org/10.1515/astro-2017-0130 |
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Article |
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doaj-54a9f7cfc823456689d752f14ac0561c2021-09-06T19:40:11ZengDe GruyterOpen Astronomy2543-63762016-09-0125327527910.1515/astro-2017-0130astro-2017-0130Photometric Study of the Seyfert Galaxy NGC 4151Shomshekova S. A.0Kusakin A. V.1Reva I. V.2V. G. Fesenkov Astrophysical Institute, 050020, Almaty, Kamenskoye platoV. G. Fesenkov Astrophysical Institute, 050020, Almaty, Kamenskoye platoV. G. Fesenkov Astrophysical Institute, 050020, Almaty, Kamenskoye platoThe results of CCD photometry in the Johnson-Morgan BV R system for the Seyfert galaxy NGC 4151 are reported. The observations were carried out from November 15, 2013 to May 13, 2016 with the 1-m telescope of Tien-Shan Astronomical Observatory of the Fesenkov Astrophysical Institute. An analysis of the light curve of NGC 4151 shows that over the time interval considered the brightness of the object varied synchronously in the three filters with the following amplitudes: ΔB = 0.68 mag, ΔV = 1.09 mag, and ΔR = 1.81 mag.https://doi.org/10.1515/astro-2017-0130galaxies: seyfertgalaxies: individual (ngc 4151)galaxies: photometry |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Shomshekova S. A. Kusakin A. V. Reva I. V. |
| spellingShingle |
Shomshekova S. A. Kusakin A. V. Reva I. V. Photometric Study of the Seyfert Galaxy NGC 4151 Open Astronomy galaxies: seyfert galaxies: individual (ngc 4151) galaxies: photometry |
| author_facet |
Shomshekova S. A. Kusakin A. V. Reva I. V. |
| author_sort |
Shomshekova S. A. |
| title |
Photometric Study of the Seyfert Galaxy NGC 4151 |
| title_short |
Photometric Study of the Seyfert Galaxy NGC 4151 |
| title_full |
Photometric Study of the Seyfert Galaxy NGC 4151 |
| title_fullStr |
Photometric Study of the Seyfert Galaxy NGC 4151 |
| title_full_unstemmed |
Photometric Study of the Seyfert Galaxy NGC 4151 |
| title_sort |
photometric study of the seyfert galaxy ngc 4151 |
| publisher |
De Gruyter |
| series |
Open Astronomy |
| issn |
2543-6376 |
| publishDate |
2016-09-01 |
| description |
The results of CCD photometry in the Johnson-Morgan BV R system for the Seyfert galaxy NGC 4151 are reported. The observations were carried out from November 15, 2013 to May 13, 2016 with the 1-m telescope of Tien-Shan Astronomical Observatory of the Fesenkov Astrophysical Institute. An analysis of the light curve of NGC 4151 shows that over the time interval considered the brightness of the object varied synchronously in the three filters with the following amplitudes: ΔB = 0.68 mag, ΔV = 1.09 mag, and ΔR = 1.81 mag. |
| topic |
galaxies: seyfert galaxies: individual (ngc 4151) galaxies: photometry |
| url |
https://doi.org/10.1515/astro-2017-0130 |
| work_keys_str_mv |
AT shomshekovasa photometricstudyoftheseyfertgalaxyngc4151 AT kusakinav photometricstudyoftheseyfertgalaxyngc4151 AT revaiv photometricstudyoftheseyfertgalaxyngc4151 |
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1717769127283654656 |