Search Publications

Imaging of HH80-81 Jet in the Near-infrared Shock Tracers H2 and [Fe II]
DOI: 10.3847/1538-4357/aca413 Bibcode: 2023ApJ...942...76M

Vig, S.; Tej, A.; Mohan, Sreelekshmi +1 more

The HH80-81 system is one of the most powerful jets driven by a massive protostar. We present new near-infrared (NIR) line imaging observations of the HH80-81 jet in the H2 (2.122 µm) and [Fe II] (1.644 µm) lines. These lines trace not only the jet close to the exciting source but also the knots located farther away. We have…

2023 The Astrophysical Journal
eHST 3
Discovery of δ Sct components in eclipsing binary systems IQ CMa, AW men and W Vol
DOI: 10.1093/mnras/stac3345 Bibcode: 2023MNRAS.518.4180U

Ulaş, Burak; Ulusoy, Ceren

We present the first evidence on the δ Sct type pulsations of the primary components of three eclipsing binaries IQ CMa, AW Men, and W Vol in the Transiting Exoplanet Survey Satellite (TESS) field. A comprehensive investigation of the binary properties is conducted. The light curves of the systems are analysed and the frequency analyses are perfor…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Multiband optical variability of a newly discovered 12 blazars sample from 2013 - 2019
DOI: 10.1093/mnras/stad904 Bibcode: 2023MNRAS.522..767J

Gupta, Alok C.; Damljanović, Goran; Bhatta, Gopal +2 more

Here we present the first optical photometric monitoring results of a sample of 12 newly discovered blazars from the ICRF - Gaia CRF astrometric link. The observations were performed from April 2013 to August 2019 using eight telescopes located in Europe. For a robust test for the brightness and colour variability, we use Abbé criterion and F-test…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Five-minute oscillations of photospheric and chromospheric swirls
DOI: 10.1051/0004-6361/202245373 Bibcode: 2023A&A...674A.142L

Liu, Jiajia; Mathioudakis, Mihalis; Erdélyi, Robert +1 more

Context. Swirls are ubiquitous in the solar atmosphere. They are thought to be related to the excitation of different modes of magnetohydrodynamic waves and pulses, as well as spicules. However, statistical studies of their collective behaviour are rare.
Aims: We aim to study the collective as well as the individual behaviour of photospheric …

2023 Astronomy and Astrophysics
Hinode 3
Asteroseismology of the Pulsating Extremely Low-mass White Dwarf SDSS J111215.82 + 111745.0: A Model with p-mode Pulsations Consistent with the Observations
DOI: 10.3847/1538-4357/aca533 Bibcode: 2023ApJ...943..113S

Su, Jie; Li, Yan

SDSS J111215.82+111745.0 is the second pulsating extremely low-mass white dwarf discovered. Two short-period pulsations, 107.56 and 134.275 s, were detected on this star, which would be the first observed pressure mode (p-mode) pulsations observed on a white dwarf. While the two potential p-modes have yet to be confirmed, they make SDSS J111215.82…

2023 The Astrophysical Journal
Gaia 3
Coronal Abundances in an Active Region: Evolution and Underlying Chromospheric and Transition Region Properties
DOI: 10.3847/1538-4357/acb343 Bibcode: 2023ApJ...944..117T

Testa, Paola; Martínez-Sykora, Juan; De Pontieu, Bart

The element abundances in the solar corona and solar wind are often different from those of the solar photosphere, typically with a relative enrichment of elements with low first ionization potential (FIP effect). Here, we study the spatial distribution and temporal evolution of the coronal chemical composition in an active region (AR) over about …

2023 The Astrophysical Journal
Hinode IRIS 3
Stellar clustering and the kinematics of stars around Collinder 121 using Gaia DR3
DOI: 10.1093/mnras/stad1817 Bibcode: 2023MNRAS.523.5306F

Ward-Thompson, Derek; Fleming, Graham D.; Kirk, Jason M.

We study the region around Collinder 121 (Cr 121) using newly available 6D data from the Gaia DR3 catalogue. Situated in the third quadrant, near the Galactic plane, Collinder 121 lies in the region of Canis Major centred around (l, b) ≈(236°, -10°). Previous studies have suggested that the stellar associations in this region comprise an OB associ…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Suzaku and Chandra study of diffuse X-ray emission from the massive star-forming region RCW 38
DOI: 10.1093/pasj/psac100 Bibcode: 2023PASJ...75..187F

Ezoe, Yuichiro; Odaka, Hirokazu; Fukushima, Aoto

In some massive star-forming regions, diffuse X-ray emission has been observed. It can be classified as thermal emission from sub- or several-keV plasmas, non-thermal emission represented by the power law, or a mixture of them. We have studied the nearby (~1.7 kpc) young massive star-forming region RCW 38. In a previous study, non-thermal diffuse …

2023 Publications of the Astronomical Society of Japan
Suzaku 3
Hydrothermal Alteration of Ultramafic Rocks in Ladon Basin, Mars—Insights From CaSSIS, HiRISE, CRISM, and CTX
DOI: 10.1029/2022JE007223 Bibcode: 2023JGRE..12807223M

Tornabene, Livio L.; Hauber, Ernst; Mège, Daniel +21 more

The evolution of the Ladon basin has been marked by intense geological activity and the discharge of huge volumes of water from the Martian highlands to the lowlands in the late Noachian and Hesperian. We explore the potential of the ExoMars Trace Gas Orbiter/Color and Stereo Surface Imaging System color image data set for geological interpretatio…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 3
Dependence of Stellar Differential Rotation on Effective Temperature and Rotation: An Analysis from Starspot Transit Mapping
DOI: 10.3847/1538-4357/acfc1b Bibcode: 2023ApJ...956..141A

Valio, Adriana; Araújo, Alexandre

Stellar rotation is crucial for studying stellar evolution, since it provides information about age, angular momentum transfer, and magnetic fields of stars. In the case of the Sun, due to its proximity, detailed observation of sunspots at various latitudes and longitudes allows a precise estimation of the solar rotation period and its differentia…

2023 The Astrophysical Journal
CHEOPS 3