Infrared Spectroscopy of Symbiotic Stars. I. Orbits for Well-Known S-Type Systems

By F. Fekel, R. Joyce, K. Hinkle, M. Skrutskie. 2000

140 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/658df6e3baf8363d8f0afb2867b17b7f3250edd1

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In Astronomy and Astrophysics

1. B. Schaefer
2. Bing Zhang
3. Pawan Kumar

In Instrumentation

1. B. Schaefer
2. Pawan Kumar
3. Bing Zhang

Citations in the corpus

• COMPREHENSIVE PHOTOMETRIC HISTORIES OF ALL KNOWN GALACTIC RECURRENT NOVAE (2009, background): “The orbital phases (based on the ephemeris of Fekel et al. 2000) of the dip covers 1.3 orbital periods, with the dip starting at phase 0.28, the dip being deepest in the V-band at phase 0.54 (with the white dwarf being in front of the red giant), the dip ending in the V-band at phase 0.16 (after…”
• Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion (2001, background): “…Borealis with P = 227.6 days (Lines, Lines, & McFaul 1988), RS Ophiuchi with P = 460 days, (Dobrzycka & Kenyon 1994), recently revised to be P = 457 days (Fekel et al. 2000), V745 Scorpii with P =unknown, V3890 Sagittarii with P =unknown, where P is the orbital period of the binary in units of day.”