Search Publications

Dependence of the eruptive filaments dynamics on their length
DOI: 10.1093/mnras/stab3403 Bibcode: 2022MNRAS.509.5713F

Filippov, B.

We analyse numerically a model of eruption of a thin flux rope with the endpoints frozen in the photosphere. The flux rope is assumed to maintain a shape of partial current-carrying torus staying initially in equilibrium in the external dipolar magnetic field. There is an unstable equilibrium point, which can be reached by slow evolution of the sy…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 3
Improving the solar wind density model used in processing of spacecraft ranging observations
DOI: 10.1093/mnras/stac1229 Bibcode: 2022MNRAS.514.3191A

Pavlov, Dmitry; Aksim, Dan

Solar wind plasma as a cause of radio signal delay plays an important role in solar and planetary science. Early experiments studying the distribution of electrons near the Sun from spacecraft ranging measurements were designed so that the radio signal was passing close to the Sun. At present, processing of spacecraft tracking observations serves …

2022 Monthly Notices of the Royal Astronomical Society
SOHO 3
Hubble Space Telescope Captures UGC 12591: bulge/disc properties, star formation and 'missing baryons' census in a very massive and fast-spinning hybrid galaxy
DOI: 10.1093/mnras/stac2683 Bibcode: 2022MNRAS.517...99R

Mukherjee, Dipanjan; Mirakhor, Mohammad; Dhiwar, Suraj +4 more

We present Hubble Space Telescope (HST) observations of the nearby, massive, highly rotating hybrid galaxy UGC 12591, along with observations in the UV to FIRbands. HST data in V, I, and H bands is used to disentangle the structural components. Surface photometry shows a dominance of the bulge over the disc with an H-band B/D ratio of $69{{\,\rm p…

2022 Monthly Notices of the Royal Astronomical Society
eHST 3
Broad-band spectral analysis of LMXB 2S 0921-63 with Suzaku
DOI: 10.1093/mnras/stac2698 Bibcode: 2022MNRAS.517..825S

Jain, Chetana; Dutta, Anjan; Sharma, Prince

We present the broad-band spectral analysis of the low-mass X-ray binary 2S 0921-63 by using the Suzaku archival data covering the orbital phase between 0.31 and 1.16 during four close observations. It is the first time that a broad-band spectral analysis of 2S 0921-63 has been done up to 25 keV. The 0.5-10 keV XIS count rate varied between ~1 and…

2022 Monthly Notices of the Royal Astronomical Society
Suzaku 3
On the validity of the spectroscopic age indicators [Y/Mg], [Y/Al], [Y/Si], [Y/Ca], and [Y/Ti] for giant stars
DOI: 10.1093/mnras/stac1183 Bibcode: 2022MNRAS.514.4816K

Abuchaim, Yuri; Kerber, Leandro; Katime Santrich, Orlando J. +1 more

The abundance ratios [Y/Mg], [Y/Al], [Y/Si], [Y/Ca], and [Y/Ti] have been suggested as chemical clocks for solar-metallicity dwarf stars in the field as well as for giant stars in open clusters. To verify this last hypothesis, we derive these abundances ratios of 50 giant stars belonging to seven open clusters. To calculate the abundances, we anal…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Companion mass limits for 17 binary systems obtained with binary differential imaging and MagAO/Clio
DOI: 10.1093/mnras/stac2056 Bibcode: 2022MNRAS.515.4487P

Weinberger, Alycia J.; Close, Laird M.; Males, Jared R. +4 more

Improving direct detection capability close to the star through improved star subtraction and post-processing techniques is vital for discovering new low-mass companions and characterizing known ones at longer wavelengths. We present results of 17 binary star systems observed with the Magellan adaptive optics system (MagAO) and the Clio infrared c…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
A multiwavelength study of the flat-spectrum radio quasar NVSS J141922-083830 covering four flaring episodes
DOI: 10.1093/mnras/stac2181 Bibcode: 2022MNRAS.517.5791B

Stalin, C. S.; Kniazev, A.; Buckley, D. A. H. +9 more

We present multiwavelength observations and a model for flat-spectrum radio quasar (FSRQ) NVSS J141922-083830, originally classified as a blazar candidate of unknown type (BCU II object) in the Third Fermi-LAT AGN Catalog. Relatively bright flares (>3 magnitudes) were observed on 2015 February 21 (MJD 57074) and 2018 September 8 (MJD 58369) in …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Comparison of the active galactic nuclei Baldwin effect with the modified Baldwin effect of the ultraviolet-optical emission lines in a single sample
DOI: 10.1093/mnras/stac2076 Bibcode: 2022MNRAS.515.5836W

Shang, Zhaohui; Brotherton, Michael S.; Wang, Yongjiang +1 more

The inverse relationship between equivalent width (EW) of broad emission lines and the underlying continuum luminosity, known as the Baldwin effect (BE), is an important and well-studied correlation in active galactic nuclei (AGNs). However, the EW is also considered to be anticorrelated with the Eddington ratio, referred to as the modified Baldwi…

2022 Monthly Notices of the Royal Astronomical Society
eHST 2
The evolutionary state of the chemically peculiar members of the open cluster NGC 2516
DOI: 10.1093/mnras/stac1769 Bibcode: 2022MNRAS.515.3094K

Hubrig, S.; Schöller, M.; Piskunov, A. E. +1 more

We aim at establishing safe membership and evolutionary status of 11 chemically peculiar (CP) stars that are residing in the domain of the open cluster NGC 2516 and are frequently referred to as cluster members. We queried the Gaia EDR3 catalogue in an area with a radius of 1° and selected 37 508 stars brighter than G = 19 mag. The cluster members…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
XMM-Newton detection of soft time lags in the TDE candidate AT 2018fyk
DOI: 10.1093/mnrasl/slab133 Bibcode: 2022MNRAS.511L..19Z

Zhang, Wenda

In this letter, we report a tentative detection of soft time lags (i.e. variability of softer photons lags behind the variability of harder photons) in one XMM-Newton observation of the tidal disruption event (TDE) candidate AT 2018fyk while the source was in the hard spectral state. The lags are detected at $6.51\times 10^{-5}~\rm Hz$. The amplit…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2