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Spectroscopic and photometric investigations of the totally eclipsing contact binary V1320 Cas
DOI: 10.1016/j.newast.2024.102254 Bibcode: 2024NewA..11202254L

Li, Kai; Gao, Xing; Liu, Jian-Fei +4 more

We analyzed the light curve of the total eclipse contact binary V1320 Cas, obtained reliable photometric solutions, confirmed it to be a W-type contact binary with a mass ratio of 3.404 and a contact degree of 23.9%, a cool spot is discovered on the less massive component. Orbital period analysis indicates that the period of V1320 Cas is decreasin…

2024 New Astronomy
Gaia 0
An Investigation of six contact binary systems and a semi-detached one
DOI: 10.1016/j.newast.2024.102228 Bibcode: 2024NewA..11002228M

Popov, Velimir; Acerbi, Francesco; Barani, Carlo +1 more

We present a photometric analysis of six W Ursae Majoris contact binaries and one semi-detached system using multifilter CCD observations. The data were obtained with the 0.25 m Schmidt Cassegrain telescope at the observatory Stazione Astronomica Betelgeuse (SAB) in Magnago, Italy, and the 30-cm Ritchey Chretien Astrograph at the IRIDA observatory…

2024 New Astronomy
Gaia 0
Unveiling compact planetary nebulae: Broad-band survey analysis and LAMOST confirmation
DOI: 10.1016/j.newast.2024.102207 Bibcode: 2024NewA..10902207G

Gutiérrez-Soto, L. A.; Weidmann, W. A.; Faifer, F. R. +1 more

Planetary nebulae (PNe) are pivotal for advancing our knowledge of stellar evolution and galactic chemical enrichment. Recent progress in surveys and data analysis has revolutionized PN research, leading to the discovery of new objects and deeper insights into their properties. We have devised a novel photometric selection method, integrating GAIA…

2024 New Astronomy
Gaia 0
A photometric study of a total-eclipse contact binary V458 Mon
DOI: 10.1016/j.newast.2024.102250 Bibcode: 2024NewA..11102250Z

Zhu, Liying; Matekov, Azizbek; Zubairi, Ahmed Waqas +3 more

We present light curve solution of V458 Mon firstly by using the Wilson-Devinney code. The total eclipse and deep minima of the light curves of V458 Monenable us to determine reliable orbital parameters of the binary system. The solution suggests that V458 Monis a low mass ratio binary system with about 0.2 possessing a moderate degree of contact.…

2024 New Astronomy
Gaia 0
Observational constraints on modified CPL models considering non-cold dark matter
DOI: 10.1016/j.newast.2024.102259 Bibcode: 2024NewA..11202259S

Sardar, Gopal; Chakraborty, Subenoy

In the present work we consider three modified Chevallier–Polarski–Linder (CPL) models with considering non-cold dark matter in the background of homogeneous and isotropic FLRW space–time model. From the observational data set ((Pantheon+)+BAO+HST) we find that all the parameters involved in the models having equation of dark energy state ωde=ω0+ω…

2024 New Astronomy
eHST 0
Further lunar occultations results from the Trebur Observatory, 2021–24
DOI: 10.1016/j.newast.2024.102289 Bibcode: 2024NewA..11302289O

Ohlert, J. M.; Richichi, A.

Following up on our initial paper (Richichi and Ohlert, 2021), we report here on 60 lunar occultation events recorded between February 2021 and March 2024 at the Michael Adrian Observatorium. An improved version of the detector was employed for the present work. The program aims mainly at the direct measurement of the angular diameter of late-type…

2024 New Astronomy
Gaia 0
Dependence of star formation rate on different properties of molecular clouds
DOI: 10.1016/j.newast.2023.102182 Bibcode: 2024NewA..10802182M

Mondal, Ashok; Chattopadhyay, Tanuka

Properties of molecular clouds (MCs) lying in our Galaxy and their star formation scenarios have been investigated with the help of multivariate unsupervised machine learning techniques concerning several observable parameters. At first, the MCs have been classified into four coherent groups using the standard K-means clustering method. Subsequent…

2024 New Astronomy
Gaia 0
Analysis of photometric and spectroscopic variability of red supergiant Betelgeuse
DOI: 10.1016/j.newast.2022.101962 Bibcode: 2023NewA...9901962J

Jadlovský, Daniel; Krtička, Jiří; Paunzen, Ernst +1 more

Betelgeuse is a pulsating red supergiant whose brightness is semi periodically variable and in February 2020 reached a historical minimum, the Great Dimming. The aims of this study are to characterize Betelgeuse's variability based on available archival data and to study possible causes of light variability. Many spectra, from ultraviolet and opti…

2023 New Astronomy
eHST 11
A constrained cosmological model in f(R ,Lm) gravity
DOI: 10.1016/j.newast.2023.102070 Bibcode: 2023NewA..10402070S

Singh, J. K.; Shaily; Myrzakulov, Ratbay +1 more

In this article, we study the expanding nature of the universe in the context of f(R ,Lm) gravity theory, here R represents the Ricci scalar and Lm is the matter Lagrangian density. With a specific form of f(R ,Lm) , we obtain the field equations for flat FLRW metric. We parametrize the deceleration parameter in te…

2023 New Astronomy
eHST 6
DeGaPe 35: Amateur discovery of a new southern symbiotic star
DOI: 10.1016/j.newast.2022.101943 Bibcode: 2023NewA...9801943P

Charbonnel, Stéphane; Garde, Olivier; Merc, Jaroslav +6 more

In this work, we present the discovery and characterization of a new southern S-type symbiotic star, DeGaPe 35. We have obtained the low-resolution spectroscopic observations and supplemented them with the photometry from Gaia DR3 and other surveys. The optical spectra of this target show prominent emission lines, including highly ionized [Fe VII]…

2023 New Astronomy
Gaia 4