Search Publications

Investigative study of five low mass ratio semi-detached binaries
DOI: 10.1007/s10509-024-04368-6 Bibcode: 2024Ap&SS.369..105G

Stassun, Keivan G.; Parthasarathy, Mudumba; Jagirdar, Rukmini +2 more

We present the first pulsation analysis of four totally eclipsing Algol systems S Cnc, SS Cet, TW And, and VW Cyg using the latest data available from Kepler (K2), and TESS databases. Based on the characteristics observed they are classified to be oscillating eclipsing Algol binaries with primary components having

2024 Astrophysics and Space Science
eHST 0
Radio continuum emission from planetary nebulae in the Small Magellanic Cloud
DOI: 10.1007/s10509-024-04342-2 Bibcode: 2024Ap&SS.369...85A

Filipović, M. D.; Crawford, E. J.; Bojičić, I. +3 more

We report 11 new radio continuum measurements of established planetary nebulae (PNe) in the Small Magellanic Cloud (SMC) that we observed at 5.5 and 9 GHz with the Australia Telescope Compact Array (ATCA). These new radio detections are PNe with catalogued names: SMP SMC 2, SMP SMC 3, SMP SMC 5, SMP SMC 8, SMP SMC 13, SMP SMC 14, SMP SMC 19, MGPN …

2024 Astrophysics and Space Science
eHST 0
Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds
DOI: 10.1007/s10509-023-04183-5 Bibcode: 2023Ap&SS.368...24M

Mansfield, Megan

Spectroscopy of transiting exoplanets has revealed a wealth of information about their atmospheric compositions and thermal structures. In particular, studies of highly irradiated exoplanets at temperatures much higher than those found in our solar system have provided detailed information on planetary chemistry and physics because of the high lev…

2023 Astrophysics and Space Science
eHST 2
Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars
DOI: 10.1007/s10509-022-04127-5 Bibcode: 2022Ap&SS.367..124J

Hillier, D. J.; Carciofi, A. C.; Nazé, Y. +12 more

UV spectroscopy and spectropolarimetry hold the key to understanding certain aspects of massive stars that are largely inaccessible (or exceptionally difficult) with optical or longer wavelength observations. As we demonstrate, this is especially true for the rapidly-rotating Be and Bn stars, owing to their high temperatures, geometric asymmetries…

2022 Astrophysics and Space Science
eHST 18
A radio continuum study of NGC 2082
DOI: 10.1007/s10509-022-04086-x Bibcode: 2022Ap&SS.367...61B

Filipović, M. D.; Dai, S.; Barnes, L. +2 more

We present radio continuum observations of NGC 2082 using ASKAP, ATCA and Parkes telescopes from 888 MHz to 9000 MHz. Some 20 arcsec from the centre of this nearby spiral galaxy, we discovered a bright and compact radio source, J054149.24–641813.7, of unknown origin. To constrain the nature of J054149.24–641813.7, we searched for transient events …

2022 Astrophysics and Space Science
eHST 1
New H I observations of KK 69. Is KK 69 a dwarf galaxy in transition?
DOI: 10.1007/s10509-020-03825-2 Bibcode: 2020Ap&SS.365..111S

Koribalski, B. S.; Benaglia, P.; Saponara, J. +1 more

We present new H I data of the dwarf galaxy KK 69, obtained with the Giant Metrewave Radio Telescope (GMRT) with a signal-to-noise ratio almost double previous observations. We carried out a Gaussian spectral decomposition and stacking methods to identify the cold neutral medium (CNM) and the warm neutral medium (WNM) of the H I gas. We found that…

2020 Astrophysics and Space Science
eHST 4
Virial models and anisotropy of velocity dispersion in E-galaxies
DOI: 10.1007/s10509-020-3728-4 Bibcode: 2020Ap&SS.365...15K

Kondratyev, B. P.; Kireeva, E. N.

A tensor virial approach is used to construct detailed models of 22 flattened ellipticals. The models are combined with the new observational data: extended surface brightness distributions, the profiles of isophotes flattening and their twisting, the rotation curves and the velocity dispersion profiles. A key feature of these models is a rigorous…

2020 Astrophysics and Space Science
eHST 1
Local dark energy in the Sculptor Filament of galaxies
DOI: 10.1007/s10509-020-03840-3 Bibcode: 2020Ap&SS.365..120P

Pruzhinskaya, M. V.; Karachentsev, I. D.; Chernin, A. D.

Two dozens of different mass galaxies observed at distances less than 10 Mpc from the Local Group are organized in the elongated structure known as the Sculptor Filament. We use recent Hubble Space Telescope data on local galaxies to study the dynamical structure and evolutionary trends of the filament. An N-body computer model, which reproduces i…

2020 Astrophysics and Space Science
eHST 1
Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
DOI: 10.1007/s10509-019-3627-8 Bibcode: 2019Ap&SS.364..134P

Park, Chan-Gyung; Ratra, Bharat

Cosmic microwave background (CMB) anisotropy (spatial inhomogeneity) data provide the tightest constraints on the Hubble constant, matter density, spatial curvature, and dark energy dynamics. Other data, sensitive to the evolution of only the spatially homogeneous part of the cosmological model, such as Type Ia supernova apparent magnitude, baryon…

2019 Astrophysics and Space Science
eHST 86
Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
DOI: 10.1007/s10509-019-3567-3 Bibcode: 2019Ap&SS.364...82P

Park, Chan-Gyung; Ratra, Bharat

We constrain tilted spatially-flat and untilted nonflat XCDM dynamical dark energy inflation parameterizations using Planck 2015 cosmic microwave background (CMB) anisotropy data and recent baryonic acoustic oscillations distance measurements, Type Ia supernovae data, Hubble parameter observations, and growth rate measurements. Inclusion of the fo…

2019 Astrophysics and Space Science
eHST 86