IDENTIFICATION OF DQ SERPENTIS AND DT SERPENTIS AS SYMBIOTIC STARS

Authors
CIESLINSKI D STEINER JE ELIZALDE F PEREIRA MG
Citation
D. Cieslinski et al., IDENTIFICATION OF DQ SERPENTIS AND DT SERPENTIS AS SYMBIOTIC STARS, Astronomy & Astrophysics. Supplement series, 124(1), 1997, pp. 57-60
Citations number
15
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Astronomy & Astrophysics. Supplement series → ACNP
ISSN journal
03650138
Volume
124
Issue
1
Year of publication
1997
Pages
57 - 60
Database
ISI
SICI code
0365-0138(1997)124:1<57:IODSAD>2.0.ZU;2-A
Abstract
Optical and near infrared spectroscopy of the stars DQ Ser and DT Ser are presented. DQ Ser shows a late-type continuum (M3 - M5) with emiss ion lines of Balmer series, HeI, HeII, [OIII], OI and Carl triplet whi le DT Ser presents a earlier spectral type with emission of Balmer lin es, HeI, HeII and [OIII]. DT Ser is a faint V = 15.4 star 5 arcsec fro m a Tr = 12.8 G companion. We suggest it to be a yellow symbiotic star .