Search Publications

Investigation of the M13 Globular Cluster: Characteristics and Pulsation Periods of Its RR Lyrae Stars V8, V31, and V54
Bibcode: 2024JAVSO..52...43V

Wang, J.; Lee, K.; Tock, K. +2 more

Images of the Messier 13 (M13/NGC 6205) globular cluster were requested from the Las Cumbres Global Observatory's 40-centimeter telescope to investigate the chemical composition and characteristics of the cluster along with three of its RR Lyrae variable stars. Gaia Data Release 3 data were used to fit an isochrone by varying parameters such as di…

2024 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 0
Evolutionary map of the universe (EMU): Observations of filamentary structures in the Abell S1136 galaxy cluster
DOI: 10.1017/pasa.2024.36 Bibcode: 2024PASA...41...50M

Reiprich, Thomas H.; Koribalski, Bärbel S.; Norris, Ray P. +17 more

We present radio observations of the galaxy cluster Abell S1136 at 888 MHz, using the Australian Square Kilometre Array Pathfinder radio telescope, as part of the Evolutionary Map of the Universe Early Science program. We compare these findings with data from the Murchison Widefield Array, XMM-Newton, the Wide-field Infrared Survey Explorer, the D…

2024 Publications of the Astronomical Society of Australia
XMM-Newton 0
A search for Galactic post-asymptotic giant branch stars in Gaia DR3
DOI: 10.1051/0004-6361/202346330 Bibcode: 2024A&A...688A.209G

Dafonte, C.; González-Santamaría, I.; Manteiga, M. +3 more

Context. When low- and intermediate-mass stars leave the asymptotic giant branch (AGB) phase, and before they reach the planetary nebula stage, they enter a very brief and rather puzzling stellar evolutionary stage called post-AGB stage. The post-AGB phase lasts very briefly, about a few thousand years at most. The number of objects that are confi…

2024 Astronomy and Astrophysics
Gaia 0
The Redshift of GRB 190829A/SN 2019oyw: A Case Study of GRB-SN Evolution
DOI: 10.3847/1538-4357/ad8dd8 Bibcode: 2024ApJ...977..256B

Fruchter, Andrew S.; Izzo, Luca; Tanvir, Nial +7 more

The nearby long gamma-ray burst (GRB) 190829A was observed using the Hubble Space Telescope/Wide Field Camera 3/infrared grisms about four weeks to 500 days after the burst. We find the spectral features of its associated supernova, SN 2019oyw, are redshifted by several thousand km s‑1 compared to the redshift of the large spiral galaxy…

2024 The Astrophysical Journal
eHST 0
Seasonal low albedo streaks at the edge of the Martian south polar layered deposits
DOI: 10.1016/j.icarus.2023.115790 Bibcode: 2024Icar..40715790P

Lucchetti, Alice; Pajola, Maurizio; Cremonese, Gabriele +6 more

Low Albedo Streaks (LAS) are narrow dark streaks observed at the edges of the South Polar Layered Deposits (SPLD) on Mars. We investigate the seasonal morphology, surface topography of LAS-rich areas using monochrome and multiband images from both the High Resolution Imaging Science Experiment (HiRISE) and the Color and Stereo Surface Imaging Syst…

2024 Icarus
ExoMars-16 0
Possible Supercritical Accretion on the Ultraluminous X-Ray Source in the Metal-poor Galaxy I Zw 18
DOI: 10.3847/1538-4357/ad4e34 Bibcode: 2024ApJ...970....8Y

Yoneyama, Tomokage; Matsumoto, Hironori; Noda, Hirofumi +2 more

We present an analysis of X-ray observations of the ultraluminous X-ray source (ULX) in I Zw 18 based on archival data taken with Chandra, XMM-Newton, and Suzaku. This ULX is considered to be an intermediate-mass black hole candidate simply because it is in the lowest-metallicity environment among ULXs, where the formation of heavy black holes is …

2024 The Astrophysical Journal
Suzaku XMM-Newton 0
Deep Hard X-ray Survey of the M81 Field Based on INTEGRAL1 Data
DOI: 10.1134/S1063773724600115 Bibcode: 2024AstL...50...25K

Sazonov, S. Yu.; Mereminskiy, I. A.; Krivonos, R. A.

We have carried out a deep survey of the M81 field in the 25-60 keV energy band based on long-term (2003-2023) INTEGRAL observations. A record sensitivity of 0.16 mCrab at a detection significance of $4σ$ has been achieved in the central part of the field owing to the long accumulated exposure (19.2 Ms). The total area of the survey is 1004 deg${}…

2024 Astronomy Letters
INTEGRAL 0
Orbits and Dynamical Masses for Six Binary Systems in the Hyades Cluster
DOI: 10.3847/1538-4357/ad54b2 Bibcode: 2024ApJ...971...31T

Torres, Guillermo; Latham, David W.; Klement, Robert +8 more

We report long-baseline interferometric observations with the CHARA Array that resolve six previously known double-lined spectroscopic binary systems in the Hyades cluster, with orbital periods ranging from 3 to 358 days: HD 27483, HD 283882, HD 26874, HD 27149, HD 30676, and HD 28545. We combine those observations with new and existing radial-vel…

2024 The Astrophysical Journal
Gaia 0
Chemical composition of planetary hosts: C, N, and α-element abundances
DOI: 10.1051/0004-6361/202451889 Bibcode: 2024A&A...691A.160S

Tautvaišienė, G.; Mikolaitis, Š.; Minkevičiūtė, R. +4 more

Context. Accurate atmospheric parameters and chemical composition of planet hosts play a major role in characterising exoplanets and understanding their formation and evolution. Aims. Our objective is to uniformly determine atmospheric parameters and chemical abundances of carbon (C), nitrogen (N), oxygen(O), and the α-elements, magnesium (Mg) and…

2024 Astronomy and Astrophysics
Gaia 0
Broad-Band X-Ray Analysis of NGC 3227
DOI: 10.1093/ptep/ptae125 Bibcode: 2024PTEP.2024i3E01N

Newman, Jared; Tsuruta, Sachiko; Liebmann, Andrew C. +2 more

Previously in Project A we carried out analysis of the data obtained by observations of the 1.5 Seyfert galaxy NGC 3227-the two observations performed by XMM-Newton in 2000 and 2006 and six observations by Suzaku in 2008. In the current paper, Project B, our work was extended to joint XMM-Newton and NuSTAR observations in 2016 as well as a NuSTAR …

2024 Progress of Theoretical and Experimental Physics
XMM-Newton 0