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Broad-band analysis of X-ray pulsar 2S 1845-024
DOI: 10.1051/0004-6361/202141608 Bibcode: 2022A&A...657A..58N

Tsygankov, Sergey S.; Lutovinov, Alexander A.; Poutanen, Juri +4 more

We present the results of a detailed investigation of the poorly studied X-ray pulsar 2S 1845−024 based on data obtained at the NuSTAR observatory during the type I outburst in 2017. Neither pulse phase-averaged nor phase-resolved spectra of the source show evidence for a cyclotron absorption feature. We also used data obtained from other X-ray ob…

2022 Astronomy and Astrophysics
XMM-Newton 4
Deep V and I CCD photometry of young star cluster NGC 1893 with the 3.6m DOT
DOI: 10.1007/s12036-021-09785-5 Bibcode: 2022JApA...43....7P

Pandey, S. B.; Panwar, Neelam; Kumar, Amit

Young star clusters consisting of massive stars are the ideal sites to study the star formation processes and influence of massive stars on the subsequent star formation. NGC 1893 is a young star cluster associated with the HII region Sh2-236. It contains about five 'O'-type stars and several early 'B'-type stars. It is located at a moderate dista…

2022 Journal of Astrophysics and Astronomy
Gaia 4
The eROSITA extragalactic CalPV serendipitous catalog
DOI: 10.1051/0004-6361/202243362 Bibcode: 2022A&A...664A.126L

Maitra, Chandreyee; Nandra, Kirpal; Reiprich, Thomas H. +22 more

Context. The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) observatory performed calibration and performance verification (CalPV) observations between September 2019 and December 2019, ahead of the planned 4-yr all-sky surveys. Most of them were deep, pointing-mode observations.
Aims: We present here the X-ray catalog det…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 4
Unveiling the formation of NGC 2915 with MUSE: A counter-rotating stellar disk embedded in a disordered gaseous environment
DOI: 10.1051/0004-6361/202243944 Bibcode: 2022A&A...668A.179T

Lin, Zesen; Chen, Guangwen; Kong, Xu +6 more

NGC 2915 is a unique nearby galaxy that is classified as an isolated blue compact dwarf based on its optical appearance but has an extremely extended H I gas disk with prominent Sd-type spiral arms. To unveil the starburst-triggering mystery of NGC 2915, we performed a comprehensive analysis of deep VLT/MUSE integral field spectroscopic observatio…

2022 Astronomy and Astrophysics
eHST 4
On the precision of full-spectrum fitting of simple stellar populations - IV. A systematic comparison with results from colour-magnitude diagrams
DOI: 10.1093/mnras/stac566 Bibcode: 2022MNRAS.512.2014A

Goudfrooij, Paul; Asa'd, Randa; As'ad, A. M.

In this fourth paper of a series on the precision of ages of stellar populations obtained through the full-spectrum fitting technique, we present a first systematic analysis that compares the age, metallicity, and reddening of star clusters obtained from resolved and unresolved data [namely colour-magnitude diagrams (CMDs) and integrated-light spe…

2022 Monthly Notices of the Royal Astronomical Society
eHST 4
Constraining leptonic emission scenarios for the PeVatron candidate HESS J1702−420 with deep XMM-Newton observations
DOI: 10.1051/0004-6361/202244696 Bibcode: 2022A&A...667A.130G

Khélifi, B.; Lemière, A.; Terrier, R. +3 more


Aims: We aim to search for a hidden leptonic accelerator, such as a high-Ė pulsar, associated with the unidentified TeV object HESS J1702−420A.
Methods: We carried out a 72 ks X-ray observation with the XMM-Newton satellite and analyzed the resulting data jointly with the publicly available HESS spectral energy distribution (SED) results…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 4
Photometric Investigation of Contact Binary DY Cet Based on TESS Data
DOI: 10.1088/1674-4527/ac5ee8 Bibcode: 2022RAA....22e5013Y

Yıldırım, M. F.

We present a photometric analysis of the Transiting Exoplanet Survey Satellite (TESS) light curve of contact binary system DY Cet and the behavior of its orbital period variation. The light curve and published radial velocity data analysis was performed using the Wilson-Devinney code. As a result of simultaneous analysis of the light curve with ra…

2022 Research in Astronomy and Astrophysics
Gaia 4
Effects from dayside magnetosphere to distant tail unleashed by a bifurcated, non-reconnecting interplanetary current sheet
DOI: 10.3389/fphy.2022.942486 Bibcode: 2022FrP....10.2486F

Berchem, J.; Wing, S.; Farrugia, C. J. +6 more

Global magnetospheric effects resulting from the passage at Earth of large-scale structures have been well studied. The effects of common and short-term features, such as discontinuities and current sheets (CSs), have not been studied in the same depth. Herein we show how a seemingly unremarkable interplanetary feature can cause widespread effects…

2022 Frontiers in Physics
Cluster 4
Gas inflows in the polar ring of NGC 4111: the birth of an AGN
DOI: 10.1093/mnras/stac634 Bibcode: 2022MNRAS.512.2556H

Lützgendorf, Nora; Ma, Chung-Pei; Gebhardt, Karl +14 more

We have used Hubble Space Telescope (HST) images, SAURON Integral Field Spectroscopy (IFS), and adaptative optics assisted Gemini NIFS near-infrared K-band IFS to map the stellar and gas distribution, excitation and kinematics of the inner few kpc of the nearby edge-on S0 galaxy NGC 4111. The HST images map its ≈450 pc diameter dusty polar ring, w…

2022 Monthly Notices of the Royal Astronomical Society
eHST 4
Interaction of convective plasma and small-scale magnetic fields in the lower solar atmosphere
DOI: 10.1007/s41614-022-00094-0 Bibcode: 2022RvMPP...6...33V

Utz, Dominik; Vargas Domínguez, Santiago

In the following short review we will outline some of the possible interaction processes of lower solar atmospheric plasma with the embedded small-scale solar magnetic fields. After introducing the topic, important types of small-scale solar magnetic field elements are outlined to then focus on their creation and evolution, and finally end up desc…

2022 Reviews of Modern Plasma Physics
Hinode IRIS 4