Search Publications

Dissecting the Extended X-Ray Emission in the Merging Pair NGC 6240: Photoionization and Winds
DOI: 10.3847/1538-4357/ac5025 Bibcode: 2022ApJ...927..166P

Elvis, M.; Fabbiano, G.; Nardini, E. +3 more

We present a detailed spectral and imaging analysis of the central 15″ radius (~7.5 kpc) region of the merger galaxy NGC 6240 that makes use of all the available Chandra-ACIS data (0.3-3 keV effective exposure of ~190 ks). This region shows extended X-ray structures with lower-energy counterparts imaged in CO, [O III], and Hα line emission. We fin…

2022 The Astrophysical Journal
eHST 7
Orbital parameters and activity of ZZ Tau - a low-mass young binary with circumbinary disc
DOI: 10.1093/mnras/stac1798 Bibcode: 2022MNRAS.515..796B

Safonov, B.; Belinski, A.; Emelyanov, N. +5 more

We present the results of our new observations of the young binary ZZ Tau with a circumbinary disc. The system was found to consist of two coeval (age < 2 Myr) classical T Tauri stars with the total mass 0.86 ± 0.09 M, orbital period 46.8 ± 0.8 yr, semimajor axis 88.2 ± 2.1 mas, eccentricity 0.58 ± 0.02, and the orbital inclination …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
The recurrent nova U Scorpii from the 2010.1 to 2022.4 eruptions; the missed eruption of 2016.78 ± 0.10 and the critical complex period changes
DOI: 10.1093/mnras/stac2511 Bibcode: 2022MNRAS.516.4497S

Schaefer, Bradley E.

U Sco is a recurrent nova with 11 observed eruptions, most recently in 2010.1 and 2022.4. I report on my program (running since 1989) of measuring eclipse times and brightnesses of U Sco in quiescence, from 2010 to 2022. The orbital period suddenly increased by +22.4 ± 1.0 parts-per-million across the 2010.1 eruption. This period change is greater…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 7
Distributions of gas and small and large grains in the LkHα 330 disk trace a young planetary system
DOI: 10.1051/0004-6361/202243704 Bibcode: 2022A&A...665A.128P

Zhu, Z.; Ginski, C.; Rosotti, G. +13 more

Planets that are forming around young stars are expected to leave clear imprints in the distribution of the gas and dust of their parental protoplanetary disks. In this paper, we present new scattered light and millimeter observations of the protoplanetary disk around LkHα 330, using SPHERE/VLT and ALMA, respectively. The scattered-light SPHERE ob…

2022 Astronomy and Astrophysics
Gaia 7
A CHEOPS-enhanced view of the HD 3167 system
DOI: 10.1051/0004-6361/202243778 Bibcode: 2022A&A...668A..31B

Alonso, R.; Deleuil, M.; Erikson, A. +92 more

Much remains to be understood about the nature of exoplanets smaller than Neptune, most of which have been discovered in compact multi-planet systems. With its inner ultra-short period planet b aligned with the star and two larger outer planets d-c on polar orbits, the multi-planet system HD 3167 features a peculiar architecture and offers the pos…

2022 Astronomy and Astrophysics
CHEOPS Gaia eHST 7
1RXH J082623.6-505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate
DOI: 10.3847/1538-4357/ac7b25 Bibcode: 2022ApJ...934..142S

Strader, Jay; Bahramian, Arash; Chomiuk, Laura +13 more

We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a ~0.4 M K-type secondary transferring mass through a low-state accretion disk to a nonmagnetic ~0.8 M white dwarf. The secondary is overluminous for its mass and domina…

2022 The Astrophysical Journal
Gaia XMM-Newton 7
The Emptiness Inside: Finding Gaps, Valleys, and Lacunae with Geometric Data Analysis
DOI: 10.3847/1538-3881/ac961e Bibcode: 2022AJ....164..226C

Hogg, David W.; Peek, Joshua E. G.; Hunt, Jason A. S. +2 more

Discoveries of gaps in data have been important in astrophysics. For example, there are kinematic gaps opened by resonances in dynamical systems, or exoplanets of a certain radius that are empirically rare. A gap in a data set is a kind of anomaly, but in an unusual sense: instead of being a single outlier data point, situated far from other data …

2022 The Astronomical Journal
Gaia 7
Quantifying kinematic substructure in star-forming regions with statistical tests of spatial autocorrelation
DOI: 10.1093/mnras/stac1955 Bibcode: 2022MNRAS.515.2266A

Parker, Richard J.; Wright, Nicholas J.; Arnold, Becky

We investigate whether spatial-kinematic substructure in young star-forming regions can be quantified using Moran's I statistic. Its presence in young star clusters would provide an indication that the system formed from initially substructured conditions, as expected by the hierarchical model of star cluster formation, even if the cluster were sp…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Solar and interplanetary events that drove two CIR-related geomagnetic storms of 1 June 2013 and 7 October 2015, and their ionospheric responses at the American and African equatorial ionization Anomaly regions
DOI: 10.1016/j.asr.2021.12.027 Bibcode: 2022AdSpR..69.2168O

Akala, A. O.; Amaechi, P. O.; Simi, K. G. +3 more

This study investigates the sequence of solar and interplanetary events that drove the 1 June 2013 and October 2015 geomagnetic storms and how the American (68°-78oE) and African (32°-42oE) Equatorial Ionization Anomaly (EIA) regions responded to them. We constructed the EIA structures by using Total Electron Content (TEC) an…

2022 Advances in Space Research
SOHO 7
The Host Galaxy of the Recoiling Black Hole Candidate in 3C 186: An Old Major Merger Remnant at the Center of a z = 1 Cluster
DOI: 10.3847/1538-4357/ac6a58 Bibcode: 2022ApJ...931..165M

Bianchi, S.; Macchetto, F. D.; Capetti, A. +10 more

3C 186, a radio-loud quasar at z = 1.0685, was previously reported to have both velocity and spatial offsets from its host galaxy, and has been considered as a promising candidate for a gravitational wave recoiling black hole triggered by a black hole merger. Another possible scenario is that 3C 186 is in an ongoing galaxy merger, exhibiting a tem…

2022 The Astrophysical Journal
eHST 7