English
Related papers

Related papers: Gaia DR 2 data and the evolutionary status of eigh…

200 papers

Using the Gaia DR2 and EDR3 data and list of post-AGB candidates, we investigate the parallax, proper motion and binarity for twenty post-AGB stars and candidates having high radial velocities. From their Gaia distances their luminosities…

Solar and Stellar Astrophysics · Physics 2022-09-28 Wako Aoki , Tadafumi Matsuno , Mudumba Parthasarathy

The evolutionary status of 24 post-AGB stars is presented based on Gaia DR3 data. All 24 stars have parallaxes accurate to better than 3 X sigma and have RUWE values less than 1.4. Based on the Gaia DR3 distances the absolute luminosities…

Solar and Stellar Astrophysics · Physics 2022-10-04 M. Parthasarathy , Marina. Kounkel , Keivan G. Stassun

Among about 1.8 million Gaia DR2 high proper motion stars with $\mu>60$ mas/yr and moderately significant parallaxes ($\varpi>3\sigma_{\varpi}$), we have selected 109 high-speed star candidates with Galactic rest frame tangential velocities…

Solar and Stellar Astrophysics · Physics 2018-11-16 Ralf-Dieter Scholz

Several dozen hypervelocity star (HVS) candidates have been reported based on the second data release of Gaia (Gaia DR2). However, it has been proven that the radial velocities of some Gaia HVS candidates are not reliable. In this paper, we…

Solar and Stellar Astrophysics · Physics 2020-05-13 Jiao Li , Shi Jia , Yan Gao , Deng-Kai Jiang , Thomas Kupfer , Ulrich Heber , Chao Liu , Xue-Fei Chen , Zhan-Wen Han

We use Gaia Data Release 2 (DR2) to place 252 Herbig Ae/Be stars in the HR diagram and investigate their characteristics and properties. For all known Herbig Ae/Be stars with parallaxes in Gaia DR2, we collected their atmospheric parameters…

Solar and Stellar Astrophysics · Physics 2018-12-12 M. Vioque , R. D. Oudmaijer , D. Baines , I. Mendigutía , R. Pérez-Martínez

Hypervelocity stars (HVSs) unbound to the Galaxy can be formed with extreme stellar interactions. Observational evidence comes from measurements of radial velocities (RVs) of objects crossing the Galactic halo and of tangential velocities…

Astrophysics of Galaxies · Physics 2024-05-22 Ralf-Dieter Scholz

We compare the parallaxes of stars from VLBI astrometry in the literature to those in the Gaia DR2 catalog. Our full sample contains young stellar objects, evolved AGB stars, pulsars and other radio stars. Excluding AGB stars, which show…

Solar and Stellar Astrophysics · Physics 2019-05-01 Shuangjing Xu , Bo Zhang , Mark J. Reid , Xingwu Zheng , Guangli Wang

Recently Kamath et al. (2021) analysed Gaia EDR3 data of eighteen post-AGB supergiants with overabundance of s-process elements. For some of these stars in their sample they find unusually very low absolute luminosities which is not in…

Solar and Stellar Astrophysics · Physics 2021-12-21 M. Parthasarathy

AIMS: With our low-resolution spectroscopic observing program for selected blue proper motion stars, we tried to find new white dwarfs (WDs) in the solar neighbourhood. METHODS: We used the LSPM catalogue with a lower proper motion limit of…

Solar and Stellar Astrophysics · Physics 2018-11-07 R. -D. Scholz , H. Meusinger , A. Schwope , H. Jahreiß , I. Pelisoli

Results of comparison of Gaia DR2 parallaxes with data derived from a combined analysis of 2MASS (Two Micron All-Sky Survey), SDSS (Sloan Digital Sky Survey), GALEX (Galaxy Evolution Explorer), and UKIDSS (UKIRT Infrared Deep Sky Survey)…

We compared positions of the Gaia first data release (DR1) secondary data set at its faint limit with CCD positions of stars in 20 fields observed with the VLT/FORS2 camera. The FORS2 position uncertainties are smaller than one…

Instrumentation and Methods for Astrophysics · Physics 2017-10-25 P. F. Lazorenko , J. Sahlmann

HD 179821 is classified as G5 Ia star. From the IRAS colors and spectral energy distributions it was classified as a post-AGB star. But some studies classify it as a massive (30 to 19 Msun ) post-red supergiant evolving to become a Type II…

Solar and Stellar Astrophysics · Physics 2019-02-20 M. Parthasarathy , G. Jasniewicz , F. Thévenin

Accurate parallaxes from Gaia DR1 (TGAS) are combined with GALEX visual Nuv magnitudes to produce absolute Mnuv magnitudes and an ultraviolet HR diagram for a large sample of astrometric stars. A functional fit is derived of the lower…

Solar and Stellar Astrophysics · Physics 2017-09-18 Valeri V. Makarov

Combining the precise parallaxes and optical photometry delivered by Gaia's second data release (Gaia DR2) with the photometric catalogues of PanSTARRS-1, 2MASS, and AllWISE, we derive Bayesian stellar parameters, distances, and extinctions…

The Gaia data release 2 (DR2) contains $>$6000 objects with parallaxes $(Plx+3\times{e\_Plx})>50$mas placing them within 20pc from the Sun. Since the expected numbers extrapolating the well-known 10pc census are much lower, nearby Gaia…

Solar and Stellar Astrophysics · Physics 2020-05-13 Ralf-Dieter Scholz

This paper presents the first census of Galactic post-Asymptotic Giant Branch stars in the HR diagram. We combined Gaia DR3 parallax-based distances with extinction corrected integrated fluxes, and derived luminosities for a sample of 185…

Solar and Stellar Astrophysics · Physics 2022-08-17 René D. Oudmaijer , Emma R. M. Jones , Miguel Vioque

Effective temperatures and luminosities are calculated for 1,475,921 Tycho-2 and 107,145 Hipparcos stars, based on distances from Gaia Data Release 1. Parameters are derived by comparing multi-wavelength archival photometry to BT-Settl…

Solar and Stellar Astrophysics · Physics 2017-08-16 Iain McDonald , Albert A. Zijlstra , Robert A. Watson

Based on data from the ESA Gaia Data Release 2 (DR2) and several ground-based, multi-band photometry surveys we compiled an all-sky catalogue of $39\,800$ hot subluminous star candidates selected in Gaia DR2 by means of colour, absolute…

Solar and Stellar Astrophysics · Physics 2019-01-09 S. Geier , R. Raddi , N. P. Gentile Fusillo , T. R. Marsh

Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements of their parallaxes is not straightforward because of the large uncertainties introduced by their dusty envelopes, their large angular sizes, and…

Solar and Stellar Astrophysics · Physics 2022-11-09 M. Andriantsaralaza , S. Ramstedt , W. H. T Vlemmings , E. De Beck

Context. The second Gaia data release (Gaia DR2) contains high precision positions, parallaxes and proper motions for 1.3 billion sources. The resulting Hertzsprung-Russel diagram reveals fine structures all over the mass range. Aims. This…

Solar and Stellar Astrophysics · Physics 2019-01-10 C. Reylé
‹ Prev 1 2 3 10 Next ›