Search Publications

Characterization of the eclipsing post-common-envelope binary TIC 60040774
DOI: 10.1093/mnras/stac2197 Bibcode: 2022MNRAS.516.1183P

Knigge, C.; Scaringi, S.; Buckley, D. A. H. +2 more

Binaries with a white dwarf primary and a main sequence secondary can be used to test our understanding of both single and binary star evolution. A small fraction of such systems experienced a common-envelope phase from which they emerged with a relatively short orbital period. Here, we present the characterization of an eclipsing post-common-enve…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 0
New Photometric and Spectroscopic Observations of the Eclipsing Binary V2080 Cygni
DOI: 10.32023/0001-5237/72.1.4 Bibcode: 2022AcA....72...55D

Schwarzenberg-Czerny, A.; Kamiński, K.; Dimitrov, W. +7 more

We present new spectroscopic and photometric measurements of the eclipsing binary V2080 Cyg. It is a detached system with similar components and an orbital period of 4.9 d. We collected spectroscopic data with two instruments, 1.88 m DDO telescope equipped with Cassegrain spectrograph and 0.5 m PST1 connected to a fiber-fed echell\'e spectrograph.…

2022 Acta Astronomica
Gaia 0
Navigation and Orbit Estimation for New Horizons' Arrokoth Flyby: Overview, Results and Lessons Learned
DOI: 10.1007/s11214-022-00877-4 Bibcode: 2022SSRv..218...11N

Weaver, Harold A.; Kavelaars, J. J.; Gwyn, Stephen D. J. +18 more

The New Horizons mission performed a successful flyby of Arrokoth, a distant Kuiper-Belt Object, on January 1, 2019, representing the farthest planetary encounter to date. The navigation strategy and performance required to deliver the spacecraft to the desired flyby target were driven by a number of challenges including those related to Arrokoth'…

2022 Space Science Reviews
Gaia 0
Search for gamma-ray emission from a galactic supernova with the anticoincidence system of SPI
DOI: 10.1093/mnras/stac1089 Bibcode: 2022MNRAS.513.2814C

Jean, P.; Isern, J.; Bravo, E. +1 more

The detection of the very early gamma-emission of a Type Ia supernova (SNIa) could provide a deep insight on the explosion mechanism and nature of the progenitor. However, this has not been yet possible as a consequence of the expected low luminosity and the distance at which all the events have occurred up to now. An SNIa occurring in our Galaxy …

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 0
Galactic component mapping of galaxy UGC 2885 by machine learning classification
DOI: 10.1016/j.asr.2022.04.032 Bibcode: 2022AdSpR..70..229K

Holwerda, Benne W.; Barmby, Pauline; Kwik, Robin J. +1 more

Automating classification of galaxy components is important for understanding the formation and evolution of galaxies. Traditionally, only the larger galaxy structures such as the spiral arms, bulge, and disc are classified. Here we use machine learning (ML) pixel-by-pixel classification to automatically classify all galaxy components within digit…

2022 Advances in Space Research
Gaia eHST 0
Rectilinear elements of visual optical double stars: With application to the 1829 southern double star catalogue of James Dunlop
DOI: 10.1002/asna.20220018 Bibcode: 2022AN....34320018L

Letchford, Roderick R.; White, Graeme L.; Brown, Carolyn J.

The relative Rectilinear motion of optical double stars provides an important clue to the relationship of the components. We provide an objective method of confirming the optical status of double stars, and of obtaining unbiased rectilinear elements solely on data obtained from the HIPPARCOS and Gaia DR2 space missions. We apply this technique to …

2022 Astronomische Nachrichten
Gaia Hipparcos 0
The OmegaWhite survey for short-period variable stars - VI. Open clusters
DOI: 10.1093/mnras/stac802 Bibcode: 2022MNRAS.513..468T

Groot, P. J.; Ramsay, G.; Jeffery, C. S. +3 more

Using light curves with ~3 min cadence and a duration of 2 h made using the OmegaWhite survey, we present the results of a search for short-period variable stars in the field of 20 open clusters. We identified 92 variable stars in these fields. Using a range of cluster member catalogues and Gaia EDR3 data, we have determined that 10 are cluster me…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 0
Quasars' physical properties study based on the medium-band photometric survey
DOI: 10.1002/asna.20210092 Bibcode: 2022AN....34310092K

Kotov, Sergey; Dodonov, Sergey; Grokhovskaya, Aleksandra

The study is about the quasars' cosmological evolution. We used the medium-band photometric survey at the 1-m Schmidt telescope of the Byurakan Astrophysical Observatory. The HS47-22 field with an area of 2.38 square degrees has been selected. We have classified objects and composed a sample of quasars using broadband photometric data and morpholo…

2022 Astronomische Nachrichten
Gaia 0
Kinematics and interplanetary characteristics of a halo Coronal Mass Ejection: a multi-wavelength analysis
DOI: 10.1007/s10509-022-04067-0 Bibcode: 2022Ap&SS.367...40S

Ebenezer, E.; Soni, Shirsh Lata

In this paper, we present the evolution and speed expansion of a shock driven by a Coronal Mass Ejection (CME) that triggered a type II radio. We combine radio analysis with a broad range of observations taken by other ground-based and space borne observatories to track the evolution of this CME/shock from Sun to 1 AU. The Halo CME studied here oc…

2022 Astrophysics and Space Science
SOHO 0
Dippers from TESS Full-frame Images. II. Spectroscopic Characterization of Four Young Dippers
DOI: 10.3847/1538-4365/ac4e8b Bibcode: 2022ApJS..259...40K

Takita, Satoshi; Hattori, Kohei; Muto, Takayuki +9 more

Photometric monitoring by the Transiting Exoplanet Survey Satellite (TESS) has discovered not only periodic signals by transiting exoplanets but also episodic or quasiperiodic dimming around young stellar objects. The dimming mechanisms of these objects, the so-called "dippers," are thought to be related to either the accretion property or the str…

2022 The Astrophysical Journal Supplement Series
AKARI 0