Search Publications

Evidence of Continuous Reconnection along a Helmet Streamer Current Sheet Observed by WISPR on Parker Solar Probe
DOI: 10.3847/1538-4357/ad509b Bibcode: 2024ApJ...970...79L

Vourlidas, Angelos; Qiu, Jiong; Stenborg, Guillermo +5 more

Parker Solar Probe's second solar encounter from 2019 March 30 to April 11 occurred during a period when the corona had a simple magnetic structure and relatively flat heliospheric current sheet (HCS), which was in the field of view of the Wide-field Imager for Solar Probe (WISPR) throughout. The images show an almost continual flow of transient d…

2024 The Astrophysical Journal
SOHO 4
The Truncated Circumgalactic Medium of the Large Magellanic Cloud
DOI: 10.3847/2041-8213/ad8b9d Bibcode: 2024ApJ...976L..28M

Fox, Andrew J.; Lehner, Nicolas; Tumlinson, Jason +6 more

The Large Magellanic Cloud (LMC) is the nearest massive galaxy to the Milky Way (MW). Its circumgalactic medium (CGM) is complex and multiphase, containing both stripped H I structures like the Magellanic Stream and Bridge and a diffuse warm corona seen in high-ion absorption. We analyze 28 active galactic nucleus sight lines passing within 35 kpc…

2024 The Astrophysical Journal
eHST 4
PICZL: Image-based photometric redshifts for AGN
DOI: 10.1051/0004-6361/202452361 Bibcode: 2024A&A...692A.260R

Shirley, R.; Bauer, F. E.; Salvato, M. +14 more

Context. Computing reliable photometric redshifts (photo-z) for active galactic nuclei (AGN) is a challenging task, primarily due to the complex interplay between the unresolved relative emissions associated with the supermassive black hole and its host galaxy. Spectral energy distribution (SED) fitting methods, while effective for galaxies and AG…

2024 Astronomy and Astrophysics
XMM-Newton 4
Dissecting the morphology of star forming complex S193
DOI: 10.1093/mnras/stad2944 Bibcode: 2024MNRAS.527.9626P

Ojha, D. K.; Pandey, Rakesh; Sharma, Saurabh +6 more

We have studied a star-forming complex S193 using near-infrared (NIR) observations and other archival data covering optical to radio wavelengths. We identified stellar clusters in the complex using the NIR photometric data and estimated the membership and distance of the clusters. Using the mid-infrared (MIR) and far-infrared (FIR) images, the dis…

2024 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 4
Active Galactic Nucleus Properties of ∼1 Million Member Galaxies of Galaxy Groups and Clusters at z < 1.4 Based on the Subaru Hyper Suprime-Cam Survey
DOI: 10.3847/1538-4357/ad32c6 Bibcode: 2024ApJ...967...65T

Goto, Tomotsugu; Imanishi, Masatoshi; Schramm, Malte +17 more

Herein, we present the statistical properties of active galactic nuclei (AGNs) for approximately 1 million member galaxies of galaxy groups and clusters with 0.1 < cluster redshift (z cl) < 1.4 selected using the Subaru Hyper Suprime-Cam, the so-called CAMIRA clusters. In this research, we focused on the AGN power fraction (f

2024 The Astrophysical Journal
eHST 4
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
DOI: 10.1093/mnras/stae354 Bibcode: 2024MNRAS.528.5065K

Balashev, S. A.; Klimenko, V. V.; Kosenko, D. N.

We present a comprehensive study of the excitation of C I fine-structure levels along 57 sight lines in the Large and Small Magellanic Clouds (LMC and SMC). The sightlines were selected by the detection of H2 in FUSE spectra. Using archival HST/COS and HST/STIS spectra, we detected absorption of C I fine-structure levels and measured th…

2024 Monthly Notices of the Royal Astronomical Society
eHST 4
On the Properties of X-Ray Corona in Seyfert 1 Galaxies
DOI: 10.3847/1538-4357/ad8088 Bibcode: 2024ApJ...976..145P

Stalin, C. S.; Ricci, Claudio; Marchesi, S. +4 more

We carried out a uniform and systematic analysis of a sample of 112 nearby bright Seyfert 1 type active galactic nuclei, the observations of which were carried out by the Nuclear Spectroscopic Telescope Array between 2013 August and 2022 May. The main goal of this analysis is to investigate the nature of the X-ray corona in Seyfert 1 galaxies. By …

2024 The Astrophysical Journal
INTEGRAL 4
"Forbidden" stars in the eROSITA all-sky survey: X-ray emission from very late-type giants
DOI: 10.1051/0004-6361/202449181 Bibcode: 2024A&A...688A...9S

Schmitt, J. H. M. M.; Czesla, S.; Robrade, J. +4 more

We present the results of the first X-ray all-sky survey (eRASS1) performed by the eROSITA instrument aboard the Spectrum-Roentgen-Gamma (SRG) mission on X-ray emitting red giants and supergiants. Focusing on stars positioned at high galactic latitudes above 20°, we constructed a complete sample of such objects using the Gaia DR3 catalog and ident…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 4
The XUV-driven escape of the planets around TOI-431 and ν2 Lupi
DOI: 10.1093/mnras/stae1054 Bibcode: 2024MNRAS.530.3500K

Fernández Fernández, Jorge; Wheatley, Peter J.; Osborn, Ares +4 more

One of the leading mechanisms invoked to explain the existence of the radius valley is atmospheric mass-loss driven by X-ray and extreme-ultraviolet irradiation, with this process stripping the primordial envelopes of young, small planets to produce the observed bimodal distribution. We present an investigation into the TOI-431 and ν2 L…

2024 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 4
Cliff collapse on Comet 67P/Churyumov-Gerasimenko - II. Imhotep and Hathor
DOI: 10.1093/mnras/stae657 Bibcode: 2024MNRAS.529.2258D

Davidsson, Björn J. R.

Cliff collapses on Comet 67P/Churyumov-Gerasimenko expose relatively pristine nucleus matter and offer rare opportunities to characterize ice-rich comet material. Here, Microwave Instrument for Rosetta Orbiter (MIRO) observations of two collapsed or crumbling cliffs in the Imhotep and Hathor regions have been assembled. The empirical diurnal anten…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 4