- ID:
- ivo://CDS.VizieR/J/MNRAS/370/2013
- Title:
- Catalogue of close binaries
- Short Name:
- J/MNRAS/370/2013
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A catalogue of close eclipsing binary systems (detached and semidetached) with at least one of the components located in the delta Scuti region of the Cepheid instability strip is presented. The positions of the stars in the instability strip are determined by their accurate temperatures and luminosities. Observationally detected binaries (20 semidetached, four detached and one unclassified) with oscillating components were included in the catalogue as a separate table. The primaries of the oscillating Algols tend to be located near the blue edge of the instability strip. Using reliable luminosities and temperatures determined by recent photometric and spectroscopic studies, we have found that at least one or two components of 71 detached and 90 semidetached systems are located in the delta Scuti region of the Cepheid instability strip. In addition, 36 detached or semidetached systems discovered by the Hipparcos satellite were also given as a separate list. One of their components is seen in the delta Scuti region, according to their spectral type or BV colours. They are potential candidate binaries with the delta Scuti-type pulsating components which need further photometric and spectroscopic studies in better precision. This catalogue covers information and literature references for 25 known and 197 candidate binaries with pulsating components.
Number of results to display per page
Search Results
- ID:
- ivo://CDS.VizieR/J/A+A/601/A145
- Title:
- Catalogue of cluster members
- Short Name:
- J/A+A/601/A145
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The hierarchical model of structure formation is a key prediction of the {LAMBDA} cold dark matter model, which can be tested by studying the large-scale environment and the substructure content of massive galaxy clusters. We present here a detailed analysis of the clusters RXC J0225.9-4154, RXC J0528.9-3927, and RXC J2308.3-0211, as part of a sample of massive X-ray luminous clusters located at intermediate redshifts. We used a multiwavelength analysis, combining WFI photometric observations, VIMOS spectroscopy, and the X-ray surface brightness maps. We investigated the optical morphology of the clusters, we looked for significant counterparts in the residual X-ray emission, and we ran several statistical tests to assess their dynamical state. We correlated the results to define various substructure features, to study their properties, and to quantify their influence on simple dynamical mass estimators. RXC J0225.9-4154 has a bi-modal core, and two massive galaxy groups are located in its immediate surroundings; they are aligned in an elongated structure that is also detected in X-rays at the 1{sigma} level. RXC J0528.9-3927 is located in a poor environment; an X-ray centroid shift and the presence of two central BCGs provide mild evidence for a recent and active dynamical history. RXC J2308.3-0211 has complex central dynamics, and it is found at the core of a superstes-cluster. The complexity of the cluster's central dynamics reflects the richness of its large-scale environment: RXC J0225 and RXC J2308 present a mass fraction in substructures larger than the typical 5-15%, whereas the isolated cluster RXC J0528 does not have any major substructures within its virial radius. The largest substructures are found in the cluster outskirts. The optical morphology of the clusters correlates with the orientation of their BCG, and with the position of the main axes of accretion.
- ID:
- ivo://CDS.VizieR/J/A+A/645/A55
- Title:
- Catalogue of cold cores in Perseus
- Short Name:
- J/A+A/645/A55
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The complex of star-forming regions in Perseus is one of the most studied due to its proximity (about 300pc). In addition, its regions show variation in star-formation activity and age, with formation of low-mass and intermediate-mass stars. In this paper, we present analyses of images taken with the Herschel ESA satellite from 70 um to 500 um. From these images, we first constructed column density and dust temperature maps. We then identified compact cores in the maps at each wavelength, and characterised the cores using modified blackbody fits to their spectral energy distributions (SEDs): we identified 684 starless cores, of which 199 are bound and potential prestellar cores, and 132 protostars. We also matched the Herschel-identified young stars with GAIA sources to model distance variations across the Perseus cloud. We measure a linear gradient function with right ascension and declination for the entire cloud. This function is the first quantitative attempt to derive the gradient in distance across Perseus, from east to west, in an analytical form. We derived mass and temperature of cores from the SED fits. The core mass function can be modelled with a log-normal distribution that peaks at 0.82M_{sun}_ suggesting a star formation efficiency of 0.30 for a peak in the system initial mass function of stars at 0.25M_{sun}_. The high-mass tail can be modelled with a power law of slope ~-2.32, which is close to the Salpeter's value. We also identify the filamentary structure of Perseus and discuss the relation between filaments and star formation, confirming that stars form preferentially in filaments. We find that the majority of filaments with ongoing star formation are transcritical against their own internal gravity because their linear masses are below the critical limit of 16M_{sun}_/pc above which we expect filaments to collapse. We find a possible explanation for this result, showing that a filament with a linear mass as low as 8 Msun/pc can already be unstable. We confirm a linear relationship between star formation efficiency and the slope of dust probability density function, and we find a similar relationship with the core formation efficiency. We derive a lifetime for the prestellar core phase of 1.69+/-0.52Myr for the whole Perseus complex but different regions have a wide range in prestellar core fractions, suggesting that star formation began only recently in some clumps. We also derive a free-fall time for prestellar cores of 0.16Myr.
- ID:
- ivo://CDS.VizieR/J/A+A/659/A166
- Title:
- Catalogue of Cosmic Filaments
- Short Name:
- J/A+A/659/A166
- Date:
- 23 Mar 2022 15:17:04
- Publisher:
- CDS
- Description:
- In this work we present a new catalogue of cosmic filaments obtained from the latest Sloan Digital Sky Survey (SDSS) public data. In order to detect filaments, we implement a version of the Subspace-Constrained Mean-Shift algorithm that is boosted by machine learning techniques. This allows us to detect cosmic filaments as one-dimensional maxima in the galaxy density distribution. Our filament catalogue uses the cosmological sample of SDSS, including Data Release 16, and therefore inherits its sky footprint (aside from small border effects) and redshift coverage. In particular, this means that, taking advantage of the quasar sample, our filament reconstruction covers redshifts up to z=2.2, making it one of the deepest filament reconstructions to our knowledge. We follow a tomographic approach and slice the galaxy data in 269 shells at different redshift. The reconstruction algorithm is applied to 2D spherical maps. The catalogue provides the position and uncertainty of each detection for each redshift slice. The quality of our detections, which we assess with several metrics, show improvement with respect to previous public catalogues obtained with similar methods. We also detect a highly significant correlation between our filament catalogue and galaxy cluster catalogues built from microwave observations of the Planck Satellite and the Atacama Cosmology Telescope.
- ID:
- ivo://CDS.VizieR/J/MNRAS/480/2953
- Title:
- Catalogue of CP stars (HgMn, ApBp, AmFm)
- Short Name:
- J/MNRAS/480/2953
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- In this paper, we present a new catalogue of chemically peculiar (CP) stars obtained by compiling publications in which abundances of metals are provided. Our catalogue includes 428 stars for which the data were obtained through spectroscopic observations. Most of them (416) are AmFm, HgMn, and ApBp stars. We have used this compilation to proceed to a statistical overview of the abundance anomalies versus the physical parameters of the stars. Spearman's rank correlation test has been applied, and a significant number of correlations of abundance peculiarities with respect to effective temperature, surface gravity, and rotation velocity have been found. Four interesting cases are discussed in details: the Mn peculiarities in HgMn stars, the Ca correlation with respect to effective temperature in AmFm stars, the case of helium and iron in ApBp stars. Furthermore, we checked for ApBp stars using Anderson-Darling test whether the belonging to a multiple system is a determinant parameter or not for abundance peculiarities.
- ID:
- ivo://CDS.VizieR/I/209A
- Title:
- Catalogue of 2700 double stars
- Short Name:
- I/209A
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- This catalog contains a compilation of measurements of binary stars discovered by Paul Couteau between 1951 and 1993. For each star, it contains a reference number to identify the star in the catalog, the Cou number, the visual magnitudes of the components, positions for 1900, 1950, and 2000, the identification of the star in the BD or in the Carte du Ciel, the magnitude from that catalog, remarks such as the proper motion, a system to which the binary belongs or its position with respect to a neighboring BD star and for many stars, the spectral type. For each observation, the data given are the date, position angle, separation, telescope size, number of observations, and the observer. Sometimes the magnitudes estimated by the observer are also given. The present description DOES NOT replace the documents referenced above. It just provides a short format description of the files making up this catalogue.
- ID:
- ivo://CDS.VizieR/J/A+A/383/631
- Title:
- Catalogue of dust clouds in the Galaxy
- Short Name:
- J/A+A/383/631
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The file cdn.dat is an unified dust cloud catalogue of the Galaxy. Considering an initial list of approximately 6500 entries we condensed them into a cross-identified all-sky catalogue containing 5004 dust clouds.
- ID:
- ivo://CDS.VizieR/J/MNRAS/331/609
- Title:
- Catalogue of eclipsing binaries in the SMC
- Short Name:
- J/MNRAS/331/609
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- The catalogue lists 167 eclipsing binary stars in the Small Magellanic Cloud detected in the database of time-series photometry for 400000 SMC stars acquired by the Microlensing Observations in Astrophysics (MOA) project during 1997. Coordinates, ephemerides, magnitudes and light curves are presented. Thirty-five systems are new detections. The limiting magnitude is about 17.5. The majority of periods lie within the range 0.4 to 20 days; 6 systems are possibly eccentric while 14 are probably or certainly so. The majority of the newly-identified systems lie in the outer regions of the SMC.
- ID:
- ivo://CDS.VizieR/J/A+A/446/785
- Title:
- Catalogue of eclipsing variables
- Short Name:
- J/A+A/446/785
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A new catalogue of 6330 eclipsing variable stars is presented. The catalogue was developed from the General Catalogue of Variable Stars (GCVS) and its textual remarks by including recently published information about classification of 843 systems and making corresponding corrections of GCVS data. The catalogue represents the largest list of eclipsing binaries classified from observations.
- ID:
- ivo://CDS.VizieR/J/AN/334/860
- Title:
- Catalogue of eclipsing variables. Version 2
- Short Name:
- J/AN/334/860
- Date:
- 21 Oct 2021
- Publisher:
- CDS
- Description:
- A new version of the Catalogue of Eclipsing Variables is presented. The catalogue contains parameters and morphological types of light curves for some 7200 stars. Spectral classification is also given when available. Recently published information about classification of 1352 systems is included in the catalogue. The catalogue represents the largest list of eclipsing binaries with available classification.
