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Reconnaissance of Suspected Old Novae

Jeff W. Robertson et al 2000 The Astronomical Journal 119 1365-1374   doi: 10.1086/301250  Help

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Jeff W. Robertson1, R. K. Honeycutt2, T. Hillwig2, J. S. Jurcevic3 and A. A. Henden4
1 Department of Physical Sciences, Arkansas Tech University, Russellville, AR 72801-2222
2 Department of Astronomy, Swain West 319, Indiana University, Bloomington, IN 47405
3 Department of Astronomy, RLM 15.308, University of Texas, Austin, TX 78712
4 US Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002
E-mail: Jeff.Robertson@mail.atu.edu, honey@astro.indiana.edu, thillwig@astro.indiana.edu, jsj@astro.as.utexas.edu and aah@nofs.navy.mil

ABSTRACT. Several of the "blank fields" in the novae atlas by Duerbeck were imaged at the WIYN 3.5 m telescope during technical engineering and commissioning activities in 1994–1995. Several old novae have been recovered utilizing CCD photometry. Multiobject spectroscopy with the Hydra/MOS instrumentation at WIYN was also used on random stars in the fields to search for a cataclysmic variable. The old novae candidates identified include SV Ari, V465 Cyg, SS LMi, V2104 Oph, GR Ori, V529 Ori, UW Per, and UW Tri.

Key words: novae, cataclysmic variables

Print publication: Issue 3 (2000 March)
Received 1999 July 20, accepted for publication 1999 November 30

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