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NGC 2660: Gaia DR2, ASteCA and the end of controversies?
Bibcode: 2021BAAA...62...77G

Perren, G. I.; Pera, M. S.; Vázquez, R. A. +4 more

NGC 2660, an old and very compact open cluster placed at about 3 kpc from the Sun in a region of moderate absorption, has been subject of several photometric and spectroscopic studies in the past. Controversies arise in terms of its distance, age and metal content. Previous comparisons with cluster synthetic models carried out did not resolve them…

2021 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0
The Unusual Weak-line Quasar PG1407+265 and Its Foreground z 0.7 X-Ray Cluster
DOI: 10.3847/1538-4357/ac0a75 Bibcode: 2021ApJ...919...22M

McDowell, Jonathan C.; Gallo, Luigi C.; Siemiginowska, Aneta +2 more

We present new observations of the odd z = 0.96 weak-line quasar PG1407+265, and report the discovery of CXOU J140927.9+261813, a z = 0.68 X-ray cluster. Archival X-ray photometry spanning nearly four decades reveals that PG1407+265 is variable at the 1 dex level on a timescale of years. V-band variability is observed with an amplitude less than 0…

2021 The Astrophysical Journal
XMM-Newton eHST 0
Orbital eccentricities as indicators of stellar populations. II. Vertical velocity distribution from the Gaia DR2 catalogue
DOI: 10.1051/0004-6361/202140835 Bibcode: 2021A&A...652A..58C

Cubarsi, R.; Stojanović, M.; Ninković, S.

Context. In previous work, we showed how the planar and vertical eccentricities of disc stars, e and e′, could be used as indicators of the stars' kinematic populations. For a local stellar sample drawn from the Gaia DR2 catalogue, these populations were represented geometrically in the eccentricity diagram, e′2 vs. e2, appro…

2021 Astronomy and Astrophysics
Gaia 0
Impact of the Solar Wind Dynamic Pressure on the Field-Aligned Currents in the Magnetotail: Cluster Observation
DOI: 10.1029/2021JA029785 Bibcode: 2021JGRA..12629785C

Dandouras, I.; Dunlop, M. W.; Rème, H. +6 more

We statistically investigate the influence of the solar wind dynamic pressure (SW Pdyn) on the field-aligned currents (FACs) in the magnetotail with 1,492 FAC cases from July to October in 2001 and 2004, which covers 74 Cluster crossings of the plasma sheet boundary layer (PSBL) in both storm time and non-storm time. The FAC density in …

2021 Journal of Geophysical Research (Space Physics)
Cluster 0
Reducing loss of significance in the computation of Earth-based two-way Doppler observables for small body missions
DOI: 10.1088/1674-4527/21/8/191 Bibcode: 2021RAA....21..191J

Li, Fei; Ye, Mao; Barriot, Jean-Pierre +5 more

Two-way Doppler measurement is a typical Earth-based radiometric technique for interplanetary spacecraft navigation and gravity science investigation. The most widely used model for the computation of two-way Doppler observables is Moyer's differenced-range Doppler (DRD) formula, which is based on a Schwarzschild approximation of the Solar-System …

2021 Research in Astronomy and Astrophysics
Rosetta 0
Absolute parameters of young stars: PU Pup
DOI: 10.1088/1674-4527/21/10/256 Bibcode: 2021RAA....21..256E

Erdem, Ahmet; Sürgit, Derya; Budding, Edwin +2 more

We present combined photometric and spectroscopic analyses of the southern binary star PU Pup. High-resolution spectra of this system were taken at the University of Canterbury Mt. John Observatory in the years 2008 and again in 2014-2015. We find the light contribution of the secondary component to be only ~2% of the total light of the system in …

2021 Research in Astronomy and Astrophysics
Gaia Hipparcos 0
Photometric and period analysis of the eclipsing binary system V2783 Ori
DOI: 10.31577/caosp.2021.51.2.163 Bibcode: 2021CoSka..51..163B

Bulut, İ.; Bulut, A.

In this study we performed the first detailed photometric and period analysis of the recently discovered eclipsing binary star V2783 Ori. The analysis of the light curve has shown that the system is in a detached configuration, with the orbital eccentricity e = 0.274 ± 0.008. The photometric mass ratio of V2783 Ori determined from the light curve …

2021 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 0
Search for Magnetars in the Galaxy M31 as Periodic X-ray Sources Based on XMM-Newton Data
DOI: 10.1134/S1063773721010072 Bibcode: 2021AstL...47...12P

Popov, S. B.; Pshirkov, M. S.; Zolotukhin, I. Yu.

Several years ago a series of powerful millisecond radio bursts with close dispersion measures was detected toward the galaxy M31. Taking the hypothesis about the possible association of these radio bursts with a magnetar in M31 as a starting point, we have searched for periodic X-ray signal sources using data from the XMM-Newton X-ray telescope. …

2021 Astronomy Letters
XMM-Newton 0
The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z = 1
DOI: 10.3847/1538-4357/abda4c Bibcode: 2021ApJ...909...49H

Pisano, D. J.; Bershady, M. A.; Crawford, S. M. +2 more

Luminous compact blue galaxies (LCBGs) are compact, star-forming galaxies that are rarely observed in the local universe but abundant at z = 1. This increase in LCBG number density over cosmic lookback time roughly follows the increase in the star formation rate density of the universe over the same period. We use publicly available data in the CO…

2021 The Astrophysical Journal
eHST 0
Dynamics of material ejected from the Hatmehit depression and landslides on comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.pss.2021.105358 Bibcode: 2021P&SS..20905358C

Czechowski, Leszek; Kossacki, Konrad J.

In this work we investigate trajectories and regions of deposition of material ejected from depression Hatmehit on comet 67P/Churyumov-Gerasimenko. This depression, located on the lobe Head, could be a result of endogenic, possibly still ongoing, activity. We calculated trajectories of the ejecta with different initial velocities and we determined…

2021 Planetary and Space Science
Rosetta 0