Search Publications

AstroSat/UVIT Study of the Diffuse Ultraviolet Radiation in the Dwarf Galaxy Holmberg II
DOI: 10.1088/1538-3873/ad5d14 Bibcode: 2024PASP..136g4101B

Shalima, P.; Gogoi, Rupjyoti; Bordoloi, Olag Pratim +4 more

We present measurements of diffuse ultraviolet (UV) emission in the dwarf irregular galaxy Holmberg II obtained with the Ultra Violet Imaging Telescope (UVIT) instrument onboard AstroSat, India's first multiwavelength space mission. With a spatial resolution of 1.″2–1.″6, these are the highest resolution UV observations of the galaxy to date. We f…

2024 Publications of the Astronomical Society of the Pacific
Herschel 0
Escape Velocity Mass of A1063
DOI: 10.3847/1538-4357/ad3de3 Bibcode: 2024ApJ...968...35R

Miller, Christopher J.; Kremin, Anthony; Rodriguez, Alexander +1 more

We measure the radius–velocity phase-space edge profile of A1063 using galaxy redshifts from Karman et al. and Mercurio et al. Combined with a cosmological model and after accounting for interlopers and sampling effects, we infer the escape velocity profile. Using the Poisson equation, we then directly constrain the gravitational potential profile…

2024 The Astrophysical Journal
eHST 0
Constraints on the parameters of keV-scale mass annihilating dark matter obtained with SRG/ART-XC observations
DOI: 10.1103/PhysRevD.110.123026 Bibcode: 2024PhRvD.110l3026Z

Burenin, R. A.; Krivonos, R. A.; Zakharov, E. I. +2 more

In this paper we present new constraints on the velocity-independent cross section of keV-scale mass annihilating dark matter particles obtained with SRG/ART-XC after 4 full-sky surveys. These constraints are derived from observations of the Milky Way Halo, 33 Local Group spheroidal dwarf (dSph) galaxies and separately for the dSph galaxy Ursa Maj…

2024 Physical Review D
INTEGRAL 0
Classification of Wolf–Rayet Stars Using Ensemble-based Machine Learning Algorithms
DOI: 10.3847/1538-4357/ad8dda Bibcode: 2024ApJ...977..170K

Das, Ramkrishna; Bhattacharya, Rajorshi; Lewis, Megan O. +2 more

We develop a robust machine learning classifier model utilizing the eXtreme-Gradient Boosting (XGB) algorithm for improved classification of Galactic Wolf–Rayet (WR) stars based on IR colors and positional attributes. For our study, we choose an extensive data set of 6555 stellar objects (from 2MASS and AllWISE data releases) lying in the Milky Wa…

2024 The Astrophysical Journal
Gaia 0
X-Ray Observations of the Enigmatic Wolf–Rayet System θ Mus: Two's Company but Three's a Crowd
DOI: 10.3847/1538-4357/ad12cc Bibcode: 2024ApJ...961..174S

Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel +1 more

θ Mus is a remarkable spectroscopic binary (SB) consisting of a carbon-type Wolf–Rayet star and OV companion (WC6+O6–7V) in a ≈19 days orbit. In addition an O-supergiant is visually detected at a small offset of 46 mas and if gravitationally bound to the SB system would have an orbital period of many decades. θ Mus is X-ray bright and a nonthermal…

2024 The Astrophysical Journal
XMM-Newton 0
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes
DOI: 10.1007/s11207-024-02319-6 Bibcode: 2024SoPh..299...87K

Dumbović, Mateja; Temmer, Manuela; Vršnak, Bojan +3 more

We investigate the deflection and rotation behaviour of 49 Earth-directed coronal mass ejections (CMEs) spanning the period from 2010 to 2020 aiming to understand the potential influence of coronal holes (CHs) on their trajectories. Our analysis incorporates data from coronagraphic observations captured from multiple vantage points, as well as ext…

2024 Solar Physics
SOHO 0
The AllWISE Catalog as an Infrared Celestial Reference Frame in the Gaia Era
DOI: 10.3847/1538-3881/ad6dd5 Bibcode: 2024AJ....168..170L

Liu, N.; Zhu, Z.; Liu, J. -C. +3 more

The launch of Gaia in 2013 December ushered in a new era of space astrometry, allowing for fundamental reference research at an unprecedented level of precision. The international celestial reference frames in the radio band and the Gaia celestial reference frame in the optical band have been established and are consistent within several microarcs…

2024 The Astronomical Journal
Gaia 0
Retrieved atmospheric properties of the sub-stellar object VHS 1256 b with HST, VLT, and JWST spectra
DOI: 10.1051/0004-6361/202451301 Bibcode: 2024A&A...690A.357L

Zhou, Yifan; Bowler, Brendan P.; Vos, Johanna M. +3 more

Motivated by the observed ~30% variations in flux from the L7 dwarf VHS 1256 b, we subjected its time-resolved Hubble Space Telescope (HST) WFC3 spectra (measured in two epochs: 2018 and 2020), as well as medium-resolution Very Large Telescope (VLT) X-shooter and Early Release Science James Webb Space Telescope (JWST) spectra to a suite of both st…

2024 Astronomy and Astrophysics
eHST JWST 0
Kinematics of Fainst Stars of the Sco-Cen Association According to Gaia Catalog
DOI: 10.1134/S106377292470077X Bibcode: 2024ARep...68..878B

Bobylev, V. V.; Bajkova, A. T.

The kinematic properties of the Sco-Cen association have been studied using the spatial velocities of young stars. New kinematic age estimates for the three components of the association with the age of UCL and LCC being $$17.7 \pm 2.4$$ Myr and the age of US being

2024 Astronomy Reports
Gaia 0
The effect of baseline on the uncertainties of range determination performed by two-site astrometric observations. A sample case for the triangulation method: TURKSAT 3A and TURKSAT 4A
DOI: 10.1016/j.ascom.2024.100787 Bibcode: 2024A&C....4600787G

Gökay, H. G.; Özdemi̇r, S.; Bağıran, M. N. +1 more

The uncertainties in range determination depending on two-site locations for GEO satellites were calculated and shown that the uncertainty in the range depends not only on linear baseline distance between the locations but also both latitude and longitude of geographic coordinates of the sites. By taking the first observing site as fixed and chang…

2024 Astronomy and Computing
Gaia 0