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KM UMa: An Active Short-period Detached Eclipsing Binary in a Hierarchical Quadruple System
DOI: 10.3847/1538-4357/ad6df7 Bibcode: 2024ApJ...974..103M

Meng, Fangbin; Zhu, Liying; Liu, Nianping +4 more

The first detailed photometric and spectroscopic analysis of the G-type eclipsing binary KM UMa is presented, which indicates that the system is a short-period detached eclipsing binary. The radial velocity curves were calculated using the cross-correlation function method based on Large Sky Area Multi-Object Fiber Spectroscopic Telescope, Sloan D…

2024 The Astrophysical Journal
Gaia 0
Variability of the Ultraluminous X-ray Source M 74 X-1 in X-ray and Optical Ranges
DOI: 10.1134/S1990341324600753 Bibcode: 2024AstBu..79..582V

Atapin, K. E.; Vinokurov, A. S.; Solovyeva, Yu. N. +1 more

Using observations of M 74 X-1 obtained with the Chandra X-ray Observatory and the Hubble Space Telescope, we identified this source in the optical range. Analysis of other archival data allowed us to track the evolution of M 74 X-1 over two decades of observations, as well as to search for a correlation between the object's variability in the X-r…

2024 Astrophysical Bulletin
Gaia 0
Detection of Two Totally Eclipsing B-type Binaries with Extremely Low Mass Ratios
DOI: 10.3847/1538-4357/ad643b Bibcode: 2024ApJ...972..119C

Qian, Shengbang; Li, Fuxing; Zang, Lei +1 more

The detection of O- and B-type stars with extremely low-mass companions is very important for understanding the formation and evolution of binary stars. However, finding them remains a challenge because the low-mass components in such systems contribute such small flux to the total. During our search for pulsations among O- and B-type stars using …

2024 The Astrophysical Journal
Gaia 0
The Digitized First Byurakan Survey Database Late-Type Stars Candidates. New Confirmations. II
DOI: 10.1007/s10511-024-09817-2 Bibcode: 2024Ap.....67...60G

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

Three new carbon C stars was confirmed among the sample of the Late-Type Stars candidates, selected on the Digitized First Byurakan Survey (DFBS) spectral plates. The DFBS is the digitized version of the First Byurakan Survey (FBS, or Markarian survey). The FBS was the first systematic survey of the extragalactic sky. This objective-prism survey w…

2024 Astrophysics
Gaia 0
The GAPS Programme at TNG: LVIII. Two multi-planet systems with long-period substellar companions around metal-rich stars
DOI: 10.1051/0004-6361/202449456 Bibcode: 2024A&A...689A.235R

Scandariato, G.; Marzari, F.; Sozzetti, A. +20 more

Context. Due to observational biases, a large fraction of known exoplanets are short-period objects. However, the search for planets began more than 20 yr ago, and so it is already possible – with the use of a suitable dataset – to begin exploring a wider range of the parameter space, such as that encompassing long-period planets. Aims. The aim of…

2024 Astronomy and Astrophysics
Gaia 0
First deep X-ray observations of the Fermi-detected steep-spectrum source and radio-loud NLS1 galaxy 3C 286
DOI: 10.1093/mnras/stae1827 Bibcode: 2024MNRAS.533.1281Y

Komossa, S.; Grupe, D.; Kraus, A. +1 more

A well-known calibrator source in radio astronomy, 3C 286 ($z=0.85$), is a compact steep-spectrum (CSS) radio source and spectroscopically classified as a narrow-line Seyfert 1 (NLS1) galaxy. It is also known for its damped Ly $\alpha$ system from an intervening galaxy at $z=0.692$ detected in both ultraviolet (UV) and radio spectra. In addition, …

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
X Persei: A study on the origin of its high-energy emission
DOI: 10.1051/0004-6361/202348835 Bibcode: 2024A&A...689A.186R

Fiocchi, M.; Natalucci, L.; Rodi, J.

Aims. The origin of the hard X-ray emission in the Be/X-ray binary system X Persei has long been debated as its atypical 'two-hump' spectrum can be modelled in multiple ways. The main debate focuses on the the high-energy hump, which is fit as either a cyclotron resonance scatter frequency (CRSF) or inverse Comptonization due to bulk Comptonizatio…

2024 Astronomy and Astrophysics
Gaia INTEGRAL 0
High-resolution Observations of Clustered Dynamic Extreme-Ultraviolet Bright Tadpoles Near the Footpoints of Corona Loops
DOI: 10.1088/1674-4527/ad8a09 Bibcode: 2024RAA....24l5010W

Chitta, L. P.; Wang, Rui; Liu, Ying D. +2 more

An extreme ultraviolet (EUV) close-up view of the Sun offers unprecedented detail of heating events in the solar corona. Enhanced temporal and spatial images obtained by the Solar Orbiter during its first science perihelion enabled us to identify clustered EUV bright tadpoles (CEBTs) occurring near the footpoints of coronal loops. Combining SDO/AI…

2024 Research in Astronomy and Astrophysics
SolarOrbiter 0
Probing the Galactic Halo with RR Lyrae Stars. VI. The Radial Velocity Curve Templates of RRc Stars
DOI: 10.1088/1674-4527/ad50b5 Bibcode: 2024RAA....24g5009H

Fang, Min; Tian, Haijun; Shi, Jianrong +8 more

We present radial velocity (RV) curve templates of RR Lyrae first-overtone (RRc) stars constructed with the Mg I b triplet and Hα lines using time-domain Medium-Resolution Survey spectra of seven RRc stars from Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 9. Additionally, we derive the relation between the stella…

2024 Research in Astronomy and Astrophysics
Gaia 0
Comment on Ádám et al. (2023): Large fraction of already known systems reported
DOI: 10.1051/0004-6361/202450463 Bibcode: 2024A&A...688A..41Z

Zasche, P.

In this work, I report that large fraction of stars detected by Ádám et al. (2023, A&A, 674, A170) and noted in that work as new discoveries are in fact known systems. This is especially true for the dense bulge fields with large blending of nearby sources. Among the published 245 stars determined to be doubly eclipsing (i.e. containing two ec…

2024 Astronomy and Astrophysics
Gaia 0