Please use this identifier to cite or link to this item:
https://www.um.edu.mt/library/oar/handle/123456789/57469| Title: | The disappearance and reappearance of optical emission lines and the drop in a Swift/XRT count rate during the recent rebrightening of TCP J21040470+4631129 |
| Authors: | Neustroev, V. Boyd, D. Sims, F. Page, K. L. Tordai, T. Brincat, Stephen M. Galdies, Charles Sjoberg, G. Zharikov, S. Osborne, J. P. Kuin, N. P. M. Marsh, T. R. Gaensicke, B. T. Knigge, C. |
| Keywords: | Dwarf novae Stars -- Classification Stars -- Observations Photometry |
| Issue Date: | 2019 |
| Publisher: | Robert E. Rutledge |
| Citation: | Neustroev, V., Boyd, D., Sims, F., Page, K. L., Tordai, T., Brincat, S. M.,... Knigge, C. (2019). The disappearance and reappearance of optical emission lines and the drop in a Swift/XRT count rate during the recent rebrightening of TCP J21040470+4631129. The Astronomer's Telegram, 13297, 13646. |
| Abstract: | We report the results of our continuing optical and X-ray monitoring of the bright WZ Sge-type dwarf nova TCP J21040470+4631129 (hereafter TCP2104) discovered on July 12, 2019 (for previous reports, see ATel #12947, #13009). Our optical photometric observations are mostly performed using 30-cm class telescopes, while spectroscopic data are obtained with the 2.1-m telescope at the OAN-SPM, the 2.5-m Isaac Newton Telescope on La Palma, and other smaller telescopes. |
| URI: | https://www.um.edu.mt/library/oar/handle/123456789/57469 |
| Appears in Collections: | Scholarly Works - InsESEMP |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| The_disappearance_and_reappearance_of_optical_emission_lines.pdf | 493.12 kB | Adobe PDF | View/Open |
Items in OAR@UM are protected by copyright, with all rights reserved, unless otherwise indicated.