The Ultraviolet Spectra of Active Galaxies WIth Double-Peaked Balmer Emission Lines

Michael Eracleous; Karen T. Lewis; J. P. Halpern; Alexei V Filippenko; Thaisa Storchi‐Bergmann; Mario Livio; A. S. Wilson

Discussion(0)

No comments yet. Be the first to comment.

Related publications

Article2016

The Ultraviolet Spectra of Active Galaxies With Double-Peaked Emission Lines

Michael Eracleous, J. P. Halpern, Thaisa Storchi‐Bergmann, Alexei V Filippenko

Article2025

A post-common-envelope binary with double-peaked Balmer emission lines from TMTS

Qichun Liu, Xiaofeng Wang, Jie Lin, Chengyuan Wu, Chunqian Li, Alexei V Filippenko, Thomas G. Brink, Yi Yang, WeiKang Zheng, Cheng Liu, Cuiying Song, Mikhail Kovalev, Hongwei Ge, Fenghui Zhang, Xiaobin Zhang, Qiqi Xia, Haowei Peng, Gaobo Xi, Jun Mo, Shengyu Yan, Jianrong Shi, Jiangdan Li, Tuan Yi

Article1995

The variability of the double-peaked Balmer lines in the active nucleus of NGC 1097

Thaisa Storchi‐Bergmann, Michael Eracleous, Mario Livio, A. S. Wilson, Alexei V Filippenko, J. P. Halpern

Article2004

Monitoring the profile variability of the double-peaked Balmer lines in Arp 102B

Suvi Gezari, J. P. Halpern, Michael Eracleous, Alexei V Filippenko

Article1995

HST Ultraviolet Spectrum of ARP 102B, the Prototypical Double-Peaked Emission-Line AGN

Michael Eracleous, Alexei V Filippenko, J. P. Halpern, K. Chen