RAMSES II - RAMan Search for Extragalactic Symbiotic Stars. Project concept, commissioning, and early results from the science verification phase
arXiv:1903.03225 · doi:10.3847/1538-3881/ab0cf7
Abstract
Symbiotic stars (SySts) are long-period interacting binaries composed of a hot compact star, an evolved giant star, and a tangled network of gas and dust nebulae. They represent unique laboratories for studying a variety of important astrophysical problems, and have also been proposed as possible progenitors of SNIa. Presently, we know 257 SySts in the Milky Way and 69 in external galaxies. However, these numbers are still in striking contrast with the predicted population of SySts in our Galaxy. Because of other astrophysical sources that mimic SySt colors, no photometric diagnostic tool has so far demonstrated the power to unambiguously identify a SySt, thus making the recourse to costly spectroscopic follow-up still inescapable. In this paper we present the concept, commissioning, and science verification phases, as well as the first scientific results, of RAMSES II - a Gemini Observatory Instrument Upgrade Project that has provided each GMOS instrument at both Gemini telescopes with a set of narrow-band filters centered on the Raman OVI 6830 A band. Continuum-subtracted images using these new filters clearly revealed known SySts with a range of Raman OVI line strengths, even in crowded fields. RAMSES II observations also produced the first detection of Raman OVI emission from the SySt LMC 1 and confirmed Hen 3-1768 as a new SySt - the first photometric confirmation of a SySt. Via Raman OVI narrow-band imaging, RAMSES II provides the astronomical community with the first purely photometric tool for hunting SySts in the local Universe.
arXiv comment23 pages, 16 figures, 5 tables, accepted for publication in AJ
References in corpus (41)
- Dwarf Galaxies of the Local Group
- The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617
- Evolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models
- The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0
- Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
- SkyMapper Southern Survey: First Data Release (DR1)
- A catalogue of symbiotic stars
- PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor
- Symbiotic stars in X-rays
- A multi-epoch spectrophotometric atlas of symbiotic stars
- A census of symbiotic stars in the 2MASS, WISE and Gaia surveys
- IPHAS and the symbiotic stars. I. Selection method and first discoveries
- SU Lyncis, a hard X-ray bright M giant: Clues point to a large hidden population of symbiotic stars
- A machine learning approach for identification and classification of symbiotic stars using 2MASS and WISE
- Population Synthesis for Symbiotic X-ray Binaries
- First detection and characterization of symbiotic stars in M31
- The Bochum Survey of the Southern Galactic Disk: II. Follow-up measurements and multi-filter photometry for 1323 square degrees monitored in 2010-2015
- Distinguishing between symbiotic stars and planetary nebulae
- Early evolution of the extraordinary Nova Del 2013 (V339 Del)
- Deep spectroscopy of the emission-line populations in NGC185
- Discovery of carbon-rich Miras in the Galactic bulge
- A Survey of the Local Group of Galaxies for Symbiotic Binary Stars. I. First detection of symbiotic stars in M33
- Discovery of Raman-scattered lines in the massive luminous emission-line star LHA 115-S 18
- Discovery of true, likely and possible symbiotic stars in the dwarf spheroidal NGC 205
- The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia
- Symbiotic Stars in OGLE Data I. Large Magellanic Cloud Systems
- Early X-ray emission from Type Ia supernovae originating from symbiotic progenitors or recurrent novae
- Centre Shift of the Raman Scattered He II 4850 in the Symbiotic Star V1016 Cygni
- Discovery of a giant, highly-collimated jet from Sanduleak's star in the Large Magellanic Cloud
- SU Lyn: diagnosing the boundary layer with UV and hard X-ray data
- The spectroscopic evolution of the symbiotic star AG Draconis. I.The O VI Raman, Balmer, and helium emission line variations during the outburst of 2006-2008
- An Extreme High-Velocity Bipolar Outflow in the Pre-Planetary Nebula IRAS 08005-2356
- Raman Scattered He II 6545 Line in the Symbiotic Star V1016 Cygni
- On the Raman O VI and related lines in classical novae
- Mass-loss rate by the Mira in the symbiotic binary V1016 Cygni from Raman scattering
- A D'-type symbiotic binary in the planetary nebula SMP LMC 88
- A Profile Analysis of Raman-scattered O VI Bands at 6825 Å and 7082 Å in Sanduleak's Star
- Quantitative Method for the Optimal Subtraction of Continuum Emission from Narrow-band Images : Skewness Transition Analysis
- Raman Scattered Ne VII973 at 4881 Å in the Symbiotic Star V1016 Cygni
- A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 Å and 7082 Å in Symbiotic Stars
- CXO J004318.8+412016, a steady supersoft X-ray source in M 31
Cited by in corpus (8)
- The GALAH Survey and Symbiotic Stars. I. Discovery and follow-up of 33 candidate accreting-only systems
- Symbiotic stars in the era of modern ground- and space-based surveys
- Discovery of five new Galactic symbiotic stars in the VPHAS+ survey
- On the absence of symbiotic stars in globular clusters
- Where are the missing symbiotic stars? Uncovering hidden Symbiotic Stars in public catalogues
- J-PLUS: Tools to identify compact planetary nebulae in the Javalambre and southern photometric local universe surveys
- Optical and X-ray studies of Be/X-ray binary 1A 0535+262 during its 2020 giant outburst
- LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit