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M dwarfs found in the first Byurakan spectral sky survey database. Gaia EDR3 and TESS data. Some preliminary results
DOI: 10.1017/pasa.2023.20 Bibcode: 2023PASA...40...23G

Gigoyan, K. K.; Gigoyan, K. S.; Kostandyan, G. R. +5 more

In order to gain more information on the 236 M dwarfs identified in the First Byurakan Survey (FBS) low-resolution (lr) spectroscopic database, Gaia EDR3 high-accuracy astrometric and photometric data and Transiting Exoplanet Survey Satellite (TESS) data are used to characterise these M dwarfs and their possible multiplicity. Among the sample of 2…

2023 Publications of the Astronomical Society of Australia
Gaia 0
A Search for Low-amplitude Periodic Brightness Variations in HD 168 443
DOI: 10.1134/S0016793223080054 Bibcode: 2023Ge&Ae..63.1277B

Bondar', N. I.; Shlyapnikov, A. A.

The paper presents the results of studying light curves of the star HD 168443 obtained from the ground-based and space photometric observations within the ASAS, KWS surveys, and the Hipparcos mission from 1990 to 2020. During 30 years of observations, the average annual brightness of the star remained constant within the measurement errors, the me…

2023 Geomagnetism and Aeronomy
Hipparcos 0
The Li-age relation: Calibration with open clusters and associations
DOI: 10.5281/zenodo.7044661 Bibcode: 2023hsa..conf..291G

Gilmore, G.; Montes, D.; Randich, S. +6 more

In this work we used a series of open clusters and associations observed by the Gaia-ESO Survey (GES) to study the use of lithium abundances (Li I spectral line at 6708 $\angstrom$) as an age indicator for pre- and main-sequence FGKM late-type stars. Previous studies of open clusters have shown that lithium depletion is not only strongly age depen…

2023 Highlights on Spanish Astrophysics XI
Gaia 0
BV photometric observations of the flickering of the dwarf nova RX And
DOI: 10.48550/arXiv.2303.08616 Bibcode: 2023BlgAJ..39...58Z

Stoyanov, K. A.; Ivanov, V. D.; Minev, M. +3 more

We report photometry of the intranight variability of the dwarf nova RX~And in two bands ($B$ and $V$). The observations are carried out during three nights in November-December 2022 with the 50/70~cm Schmidt telescope of the Rozhen National Astronomical Observatory. The observations indicate that the amplitude of the flickering is about 0.5 mag i…

2023 Bulgarian Astronomical Journal
Gaia 0
Apsidal motion and absolute parameters of GV Nor and V881 Sco based on mid-resolution spectroscopy and TESS photometry
DOI: 10.1093/mnras/stac3738 Bibcode: 2023MNRAS.519.4699S

Erdem, Ahmet; Sürgit, Derya; Engelbrecht, Chris A. +5 more

The veracity of stellar evolution models and theoretical internal structure constants may be subjected to stringent tests by using physical parameters obtained from spectroscopic and photometric observations of eclipsing binary systems that exhibit apsidal motion. Two eclipsing binary stars from the southern hemisphere with no prior published spec…

2023 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL 0
Drop in the Hard Pulsed Fraction and a Candidate Cyclotron Line in IGR J16320-4751 Seen by NuSTAR
DOI: 10.3847/1538-4357/acd541 Bibcode: 2023ApJ...951...37B

Rahoui, F.; Tomsick, J. A.; Rodriguez, J. +10 more

We report on a timing and spectral analysis of a 50 ks NuSTAR observation of IGR J16320-4751 (= AX J1631.9-4752), a high-mass X-ray binary hosting a slowly rotating neutron star. In this observation from 2015, the spin period was 1308.8 ± 0.4 s giving a period derivative $\dot{P}\sim 2\times {10}^{-8}$ s s-1 when compared with the perio…

2023 The Astrophysical Journal
Gaia INTEGRAL XMM-Newton 0
The origin of subdwarf B stars
DOI: 10.25518/0037-9565.11190 Bibcode: 2023BSRSL..9211190A

Aubrey, Callum; Napiwotzki, Ralf

The origin of subdwarf B stars (sdBs) is unclear. Different formation channels are proposed including: close-binary evolution, helium-mixing on the red giant branch and the hot flasher scenario. Circumstantial evidence exists that sdBs can result from single star evolution in high metallicity populations. We investigate this possibility by using m…

2023 Bulletin de la Societe Royale des Sciences de Liege
Gaia 0
A redshifted excess in the broad emission lines after the flare of the γ-ray narrow-line Seyfert 1 PKS 2004−447
DOI: 10.1051/0004-6361/202245184 Bibcode: 2023A&A...672L..14H

Wolf, C.; Marziani, P.; Berton, M. +6 more

PKS 2004−447 is a narrow-line Seyfert 1 (NLS1) harbouring a relativistic jet with γ-ray emission. On 2019 October 25, the Fermi-Large Area Telescope captured a γ-ray flare from this source, offering a chance to study the broad-line region (BLR) and jet during such violent events. This can provide insights into the BLR structure and jet interaction…

2023 Astronomy and Astrophysics
Gaia 0
Insight into the Origin of Cometary Ices from Rosetta/ROSINA Mass Spectrometer Data
DOI: 10.1007/978-3-031-29003-9_30 Bibcode: 2023ASSP...59..259R

Rubin, Martin

Here we review some of the major findings of the mass spectrometer suite ROSINA on board of ESA's Rosetta spacecraft to comet 67P/Churyumov-Gerasimenko. For more than 2 years, ROSINA continuously measured the composition of the gases sublimating from the comet's nucleus. ROSINA measurements provided insight into the origin of the ices in 67P/Chury…

2023 European Conference on Laboratory Astrophysics ECLA2020. The Interplay of Dust
Rosetta 0
X-Rays Trace the Volatile Content of Interstellar Objects
DOI: 10.3847/1538-4357/ace970 Bibcode: 2023ApJ...956..121C

Wang, Q. Daniel; Cabot, Samuel H. C.; Seligman, Darryl Z.

The nondetection of a coma surrounding 1I/'Oumuamua, the first discovered interstellar object (ISO), has prompted a variety of hypotheses to explain its nongravitational acceleration. Given that forthcoming surveys are poised to identify analogs of this enigmatic object, it is prudent to devise alternative approaches to characterization. In this s…

2023 The Astrophysical Journal
XMM-Newton 0