Search Publications

Signature of a chemical spread in the open cluster M37
DOI: 10.1093/mnras/stac2512 Bibcode: 2022MNRAS.516.3631G

Salaris, M.; Bedin, L. R.; Pietrinferni, A. +2 more

Recent Gaia photometry of the open cluster M37 has disclosed the existence of an extended main sequence turn-off - like in Magellanic clusters younger than about 2 Gyr - and a main sequence that is broadened in colour beyond what is expected from the photometric errors, at magnitudes well below the region of the extended turn-off, where neither ag…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Analysis of the public HARPS/ESO spectroscopic archive. Jupiter-like planets around HD103891 and HD105779
DOI: 10.1051/0004-6361/202142612 Bibcode: 2022A&A...660A.124S

Mazeh, T.; Zucker, S.; Tal-Or, L. +3 more


Aims: We use the recently published database of radial velocities (RVs) that were derived from fifteen years of HARPS/ESO observations to search for planet candidates.
Methods: For targets with sufficient RV data, we applied an automated algorithm to identify significant periodic signals and fit a Keplerian model for orbital estimates. W…

2022 Astronomy and Astrophysics
Gaia 5
Ice Features of Low-luminosity Protostars in Near-infrared Spectra of AKARI/IRC
DOI: 10.3847/1538-4357/ac7f9f Bibcode: 2022ApJ...935..137K

Choi, Minho; Lee, Jeong-Eun; Dunham, Michael M. +8 more

We present near-infrared spectra of three low-luminosity protostars and one background star in the Perseus molecular cloud, acquired using the infrared camera on board the AKARI space telescope. For the comparison with different star-forming environments, we also present spectra of the massive protostar AFGL 7009S, where the protostellar envelope …

2022 The Astrophysical Journal
AKARI 5
Calibration of NOMAD on ESA's ExoMars Trace Gas Orbiter: Part 2 - The Limb, Nadir and Occultation (LNO) channel
DOI: 10.1016/j.pss.2021.105410 Bibcode: 2022P&SS..21805410T

Vandaele, Ann Carine; Neefs, Eddy; Aoki, Shohei +19 more

The Nadir and Occultation for MArs Discovery (NOMAD) instrument is a 3-channel spectrometer suite on the ESA ExoMars Trace Gas Orbiter. Since April 2018, when the nominal science mission began, it has been measuring the constituents of the Martian atmosphere. NOMAD contains three separate spectrometers, two of which operate in the infrared: the So…

2022 Planetary and Space Science
ExoMars-16 5
Estimation of Nitrogen-to-Iron Abundance Ratios from Low-Resolution Spectra
DOI: 10.5303/JKAS.2022.55.2.23 Bibcode: 2022JKAS...55...23K

Beers, Timothy C.; Lee, Young Sun; Masseron, Thomas +1 more

We present a method to determine nitrogen abundance ratios with respect to iron ([N/Fe]) from molecular CN-band features observed in low-resolution (R ∼ 2000) stellar spectra obtained by the Sloan Digital Sky Survey (SDSS) and the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). Various tests are carried out to check the systema…

2022 Journal of Korean Astronomical Society
Gaia 5
Collisional evolution of the trans-Neptunian region in an early dynamical instability scenario
DOI: 10.1093/mnras/stac1578 Bibcode: 2022MNRAS.514.4876B

Vincent, Jean-Baptiste; Campo Bagatin, Adriano; Benavidez, Paula G. +2 more

Any early or late dynamical instability in the outer Solar system should have left their footprint on the trans-Neptunian object (TNO) populations. Here, we study the collisional and dynamical evolution of such populations numerically by an updated version of ALICANDEP, which suitably takes into account the onset of an early dynamical instability.…

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 5
A Multiwavelength Study of the Sgr B Region: Contiguous Cloud-Cloud Collisions Triggering Widespread Star Formation Events?
DOI: 10.3847/1538-4357/ac674f Bibcode: 2022ApJ...931..155E

Fukui, Yasuo; Enokiya, Rei

The Sgr B region, including Sgr B1 and Sgr B2, is one of the most active star-forming regions in the Galaxy. Hasegawa et al. originally proposed that Sgr B2 was formed by a cloud-cloud collision (CCC) between two clouds with velocities of ~45 km s-1 and ~75 km s-1. However, some recent observational studies conflict with this…

2022 The Astrophysical Journal
Herschel 5
Call and Response: A Time-resolved Study of Chromospheric Evaporation in a Large Solar Flare
DOI: 10.3847/1538-4357/ac87a9 Bibcode: 2022ApJ...936...85S

Milligan, Ryan O.; McAteer, R. T. James; Sellers, Sean G.

We studied an X1.6 solar flare produced by NOAA Active Region 12602 on 2014 October 22. The entirety of this event was covered by RHESSI, IRIS, and Hinode/EIS, allowing analysis of the chromospheric response to a nonthermal electron driver. We derived the energy contained in nonthermal electrons via RHESSI spectral fitting and linked the time-depe…

2022 The Astrophysical Journal
Hinode IRIS 5
Populations of highly variable X-ray sources in the XMM-Newton slew survey
DOI: 10.1093/mnras/stac714 Bibcode: 2022MNRAS.512.3858L

Saxton, R. D.; Yuan, Weimin; Starling, R. L. C. +2 more

We present the identifications of a flux-limited sample of highly variable X-ray sources on long time-scales from the second catalogue of the XMM-Newton SLew survey (XMMSL2). The carefully constructed sample, comprising 265 sources (2.5 per cent) selected from the XMMSL2 clean catalogue, displayed X-ray variability of a factor of more than 10 in 0…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 5
Radial distribution of plasma at comet 67P. Implications for cometary flyby missions
DOI: 10.1051/0004-6361/202243776 Bibcode: 2022A&A...663A..42E

Henri, P.; Edberg, N. J. T.; Vigren, E. +3 more

Context. The Rosetta spacecraft followed comet 67P/Churyumov-Gerasimenko (67P) for more than two years at a slow walking pace (~1 m s−1) within 1500 km from the nucleus. During one of the radial movements of the spacecraft in the early phase of the mission, the radial distribution of the plasma density could be estimated, and the ionosp…

2022 Astronomy and Astrophysics
Rosetta 5