Search Publications

X-ray polarization observations of IC 4329A with IXPE: Constraining the geometry of X-ray corona
DOI: 10.1007/s12036-023-09981-5 Bibcode: 2023JApA...44...87P

Stalin, C. S.; Pal, Indrani; Chatterjee, Rwitika +1 more

X-ray polarimetry is a powerful tool to probe the geometry of the hot X-ray corona in active galactic nuclei (AGN). Here, we present our results on the characterization of the X-ray polarization of the radio-quiet Seyfert-type AGN IC 4329A at a redshift of z=0.…

2023 Journal of Astrophysics and Astronomy
XMM-Newton 6
Depletion of 13C in CO in the Atmosphere of Mars Suggested by ExoMars-TGO/NOMAD Observations
DOI: 10.3847/PSJ/acd32f Bibcode: 2023PSJ.....4...97A

Aoki, S.; Vandaele, A. C.; Daerden, F. +19 more

The atmosphere of Mars is mainly composed by carbon dioxide (CO2). It has been predicted that photodissociation of CO2 depletes 13C in carbon monoxide (CO). We present the carbon 13C/12C isotopic ratio in CO at 30-50 km altitude from the analysis of the solar occultation measurements taken by …

2023 The Planetary Science Journal
ExoMars-16 6
The soft X-ray background with Suzaku. II. Supervirial temperature bubbles?
DOI: 10.1093/pasj/psad073 Bibcode: 2023PASJ...75.1324S

Sato, Kosuke; Yamasaki, Noriko Y.; Matsushita, Kyoko +4 more

Observations of the hot X-ray emitting interstellar medium in the Milky Way are important for studying the stellar feedback and for understanding the formation and evolution of galaxies. We present measurements of the soft X-ray background emission for 130 Suzaku observations at 75° < l < 285° and |b| > 15°. With the standard soft X-ray b…

2023 Publications of the Astronomical Society of Japan
Suzaku 6
An HST survey of 33 T8 to Y1 brown dwarfs: NIR photometry and multiplicity of the coldest isolated objects
DOI: 10.1093/mnras/stad2870 Bibcode: 2023MNRAS.526.1783F

Anderson, Jay; Bedin, Luigi R.; Allers, Katelyn +5 more

We present results from a Hubble Space Telescope imaging search for low-mass binary and planetary companions to 33 nearby brown dwarfs with spectral types of T8-Y1. Our survey provides new photometric information for these faint systems, from which we obtained model-derived luminosities, masses, and temperatures. Despite achieving a deep sensitivi…

2023 Monthly Notices of the Royal Astronomical Society
eHST 6
Dynamical detection of a companion driving a spiral arm in a protoplanetary disk
DOI: 10.1051/0004-6361/202346305 Bibcode: 2023A&A...675L...1X

Dong, Ruobing; Ren, Bin B.; Wagner, Kevin +6 more

Radio and near-infrared observations have observed dozens of protoplanetary disks that host spiral arm features. Numerical simulations have shown that companions may excite spiral density waves in protoplanetary disks via companion-disk interaction. However, the lack of direct observational evidence for spiral-driving companions poses challenges t…

2023 Astronomy and Astrophysics
Gaia 6
Photometric determination of the mass accretion rates of pre-main-sequence stars. VII. The low-density cluster NGC 376 in the Small Magellanic Cloud
DOI: 10.1051/0004-6361/202142838 Bibcode: 2023A&A...675A.203T

Panagia, Nino; De Marchi, Guido; Tsilia, Styliani


Aims: We study the properties of low-mass stars recently formed in the field of the NGC 376 cluster in the Small Magellanic Cloud (SMC).
Methods: Using photometric observations acquired with the Hubble Space Telescope (HST) in the V, I, and Hα bands, we identify 244 candidate pre-main-sequence (PMS) stars showing Hα excess emission at th…

2023 Astronomy and Astrophysics
eHST 6
A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere
DOI: 10.3847/1538-4357/acd84e Bibcode: 2023ApJ...953..133K

Oughton, Sean; Fichtner, Horst; Kleimann, Jens +1 more

We present a time-dependent, three-dimensional single-fluid model for the transport of magnetohydrodynamic (MHD) turbulence that is self-consistently evolving with a dynamic large-scale solar wind in the outer heliosphere. The emphasis is on the region beyond the termination shock, where the solar wind expands subsonically, as well as sub-Alfvénic…

2023 The Astrophysical Journal
Ulysses 6
J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
DOI: 10.1051/0004-6361/202244759 Bibcode: 2023A&A...671A..71H

Hernández-Monteagudo, C.; Hernán-Caballero, A.; Mendes de Oliveira, C. +28 more

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will observe approximately one-third of the northern sky with a set of 56 narrow-band filters using the dedicated 2.55 m Javalambre Survey Telescope (JST) at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera, in order to demonstrat…

2023 Astronomy and Astrophysics
eHST JWST 6
The Gaia view of the Cepheus OB2 association
DOI: 10.1093/mnras/stad027 Bibcode: 2023MNRAS.520.1390S

Ábrahám, Péter; Kun, Mária; Szilágyi, Máté +1 more

OB associations, birthplaces of the most luminous stars, are key objects for understanding the formation of high-mass stars and their effects on their environments. The aim of this work is to explore the structure and kinematics of the Cepheus OB2 association and characterize the history of star formation in the region - in particular, the role of…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
A Search for Unbound Stellar Companions to Pulsar J1124-5916
DOI: 10.1093/mnras/stac2616 Bibcode: 2023MNRAS.519.3865K

Kochanek, C. S.

We searched for and found no higher mass (${\gtrsim}3{\rm M}_\odot$) unbound binary stellar companions to the progenitor of pulsar J1124-5916. There are lower mass candidates, but they all have high probabilities of being false positives. There are no candidates for it now being a fully unbound triple system. Even if one of the lower mass candidat…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6