J/A+A/626/A20       MONOS. I. Spectral classifications   (Maiz Apellaniz+, 2019)

MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects. Maiz Apellaniz, J., Trigueros Paez E., Negueruela I., Barba R.H., Simon-Diaz S., Lorenzo J., Sota A., Gamen R.C., Farina C., Salas J., Caballero J.A., Morrell N.I., Pellerin A., Alfaro E.J., Herrero A., Arias J.I., Marco A. <Astron. Astrophys. 626, A20 (2019)> =2019A&A...626A..20M 2019A&A...626A..20M (SIMBAD/NED BibCode)
ADC_Keywords: Positional data ; Binaries, eclipsing ; Binaries, spectroscopic ; Spectroscopy ; Stars, O ; Surveys Keywords: stars: kinematics and dynamics - stars: early-type - binaries: general Abstract: Multiplicity in massive stars is a key element to understand the chemical and dynamical evolution of galaxies. Among massive stars, those of O type play a crucial role due to their high masses and short lifetimes. MONOS (Multiplicity Of Northern O-type Spectroscopic systems) is a project designed to collect information and study O-type spectroscopic binaries with δ>20°. In this first paper we describe the sample and provide spectral classifications and additional information for objects with previous spectroscopic and/or eclipsing binary orbits. In future papers we will test the validity of previous solutions and calculate new spectroscopic orbits. The spectra in this paper have two sources: the Galactic O-Star Spectroscopic Survey (GOSSS), a project that is obtaining blue-violet R∼2500 spectroscopy of thousands of massive stars, and LiLiMaRlin, a library of libraries of high-resolution spectroscopy of massive stars obtained from four different surveys (CAFE-BEANS, OWN, IACOB, and NoMaDS) and additional data from our own observing programs and public archives. We also use lucky images obtained with AstraLux. We present homogeneous spectral classifications for 92 O-type spectroscopic multiple systems and ten optical companions, many of them original.We discuss the visual multiplicity of each system with the support of AstraLux images and additional sources. For eleven O-type objects and for six B-type objects we present their first GOSSS spectral classifications. For two known eclipsing binaries we detect double absorption lines (SB2) or a single moving line (SB1) for the first time, to which we add a third system already reported by us recently. For two previous SB1 systems we detect their SB2 nature for the first time and give their first separate spectral classifications, something we also do for a third object just recently identified as a SB2. We also detect nine new astrometric companions and provide updated information on several others. We emphasize the results for two stars: for σ Ori AaAbB we provide spectral classifications for the three components with a single observation for the first time thanks to a lucky spectroscopy observation obtained close to the Aa,Ab periastron and for θ1 Ori CaCb we add it to the class of Galactic Of?p stars, raising the number of its members to six. Our sample of O-type spectroscopic binaries contains more triple- or higher-order systems than double systems. Description: File tablea2.dat gives the coordinates and spectral classifications for 92 O-type spectroscopic multiple systems and ten optical companions. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea2.dat 181 102 Coordinates and spectral classifications refs.dat 69 29 References -------------------------------------------------------------------------------- See also: III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014) Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- Name Object name 18- 32 A15 --- ID GOS ID of the star or main component 34- 35 I2 h RAh Right Ascension (J2000) 37- 38 I2 min RAm Right Ascension (J2000) 40- 45 F6.3 s RAs Right Ascension (J2000) 47 A1 --- DE- Declination sign (J2000) 48- 49 I2 deg DEd Declination (J2000) 51- 52 I2 arcmin DEm Declination (J2000) 54- 58 F5.2 arcsec DEs Declination (J2000) 60- 69 A10 --- SBS Spectroscopic binarity status 71- 76 A6 --- STGOSSS GOSSS spectral type 78- 83 A6 --- LCGOSSS GOSSS luminosity class 85- 94 A10 --- qualGOSSS GOSSS qualifier 96-120 A25 --- secGOSSS GOSSS secondary (+tertiary) spectral type 122-125 A4 --- refGOSSS GOSSS reference code 127-132 A6 --- STalt Alternate spectral type 134-139 A6 --- LCalt Alternate luminosity class 141-150 A10 --- qualalt Alternate qualifier 152-176 A25 --- secalt Alternate secondary (+tertiary) spectral type 178-181 A4 --- refalt Alternate reference code -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Ref Reference code 7- 25 A19 --- BibCode BibCode 27- 47 A21 --- Aut Author's name 49- 69 A21 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Jesus Maiz Apellaniz, jmaiz(at)cab.inta-csic.es
(End) Patricia Vannier [CDS] 03-May-2019
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