
Spectroscopic observations of emission-line objects at Bosscha Observatory
Author(s) -
M. Rafif Rabbani,
Azlizan Adhyaqsa,
Dimas A. Prabowo,
Aprilia,
L. Puspitarini,
Hakim L. Malasan
Publication year - 2020
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1523/1/012018
Subject(s) - spectrograph , physics , stars , observatory , astrophysics , telescope , emission spectrum , variable star , astronomy , line (geometry) , spectral line , h alpha , geometry , mathematics
We report an optical spectroscopic observational program of emission-line objects at Bosscha Observatory. The observations were conducted on 18 nights between May to July 2019. We employ the spectrograph NEO-R1000 ( R ∼1000) equipped with SBIG ST-8 XME CCD camera attached to a 28 cm ( F /10) telescope and the spectrograph LHIRES III ( R ∼5000) equipped with SBIG ST-402 CCD camera attached to a 25 cm ( F /10) telescope. Data reduction has been carried out using longslit transform routines within the Image Reduction and Analysis Facility (IRAF). We have successfully obtained the spectra of 9 Wolf-Rayet (WR) stars, 13 B-emission (Be) stars, 2 Luminous Blue Variable (LBV) stars, 8 Herbig Ae/Be (HAeBe) stars, and 1 recurrent nova. The obtained spectra are presented and discussed in this paper.