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Optical observations and dust modelling of comet 156P/Russell-LINEAR
DOI: 10.1016/j.icarus.2022.115042 Bibcode: 2022Icar..38315042A

Aravind, K.; Halder, Prithish; Ganesh, Shashikiran +5 more

Comet 156P/Russell-LINEAR is a short period Jupiter family comet with an orbital period of 6.44 years. The results from spectroscopic, photometric, polarimetric observations and dust modelling studies are presented here. From the spectroscopic study, strong emissions from CN(Δν = 0) , C3 (λ 4050 Å), C2(Δν = + 1) and C2

2022 Icarus
Rosetta 5
Spectroscopy of an extreme [O III] emitting active galactic nucleus at z = 3.212: implications for the reionization era
DOI: 10.1093/mnras/stab3279 Bibcode: 2022MNRAS.509.3102T

Feltre, Anna; Charlot, Stéphane; Shapley, Alice E. +4 more

Reionization-era galaxies often display intense nebular emission lines, both in rest-frame optical ([O III] + H β) and ultraviolet (UV; C III], C IV). How such strong nebular emission is powered remains unclear, with both active galactic nuclei (AGNs) and hot stars considered equally viable. The UV continuum slopes of these early systems tend to b…

2022 Monthly Notices of the Royal Astronomical Society
eHST 5
Searching the SETI Ellipsoid with Gaia
DOI: 10.3847/1538-3881/ac82ea Bibcode: 2022AJ....164..117D

Davenport, James R. A.; Siemion, Andrew P. V.; Cody, Ann Marie +4 more

The search for extraterrestrial intelligence (SETI) Ellipsoid is a geometric method for prioritizing technosignature observations based on the strategy of receiving signals synchronized to conspicuous astronomical events. Precise distances to nearby stars from Gaia makes constraining Ellipsoid crossing times possible. Here we explore the utility o…

2022 The Astronomical Journal
Gaia 5
The spatial evolution of young massive clusters. III. Effect of the Gaia filter on 2D spatial distribution studies
DOI: 10.1051/0004-6361/202140902 Bibcode: 2022A&A...659A..72B

Buckner, Anne S. M.; Khorrami, Zeinab; González, Marta +3 more

Context. With the third release of the high-precision optical-wavelength Gaia survey, we are in a better position than ever before to study young clusters. However, Gaia is limited in the optical down to G ∼ 21 mag, and therefore it is essential to understand the biases introduced by a magnitude-limited sample on spatial distribution studies.

2022 Astronomy and Astrophysics
Gaia 5
The Population of Compact Radio Sources in M17
DOI: 10.3847/1538-3881/ac67ec Bibcode: 2022AJ....163..276Y

Menten, Karl M.; Rodríguez, Luis F.; Loinard, Laurent +7 more

We present a catalog of radio sources of the M17 region based on deep X-band radio observations centered at 10 GHz obtained with the Jansky Very Large Array in the A configuration. We detect a total of 194 radio sources, 12 of them extended and 182 compact. We find that a significant fraction (at least 40% in our catalog) have suspected gyrosynchr…

2022 The Astronomical Journal
Gaia Herschel 5
Discovery of a Filamentary Synchrotron Structure Connected to the Coherent Magnetic Field in the Outer Galaxy
DOI: 10.3847/1538-4357/ac9b58 Bibcode: 2022ApJ...941....6W

Ricci, R.; Safi-Harb, S.; Kothes, R. +9 more

Using data from the Galactic Arecibo L-band Feed Array Continuum Transit Survey, we report the discovery of two previously unidentified, very compressed, thin, and straight polarized filaments approximately centered at Galactic coordinates, (l, b) = (182.°5, - 4.°0), which we call G182.5-4.0. Using data from the Isaac Newton Telescope Galactic Pla…

2022 The Astrophysical Journal
Gaia 5
The origin of the high-mass X-ray binary 4U 2206+54/BD+532790
DOI: 10.1093/mnras/stac184 Bibcode: 2022MNRAS.511.4123H

Neuhäuser, R.; Mugrauer, M.; Stoyanov, K. A. +7 more

Based on the Gaia EDR3 astrometric parameters and our new systemic radial velocity of the high-mass X-ray binary 4U 2206+54/BD+532790, we studied the trace back motion of the system and propose that it originated in the subgroup of the Cepheus OB1 association (Age ~4-10 Myr) with its brightest star, BD+532820 (B0V; ${\cal L}$~104.7${\ca…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
A rare phosphorus-rich star in an eclipsing binary from TESS
DOI: 10.1051/0004-6361/202142124 Bibcode: 2022A&A...658A.105F

Kama, Mihkel; Folsom, Colin P.; Eenmäe, Tõnis +6 more

Context. Few exoplanets around hot stars with radiative envelopes have been discovered, although new observations from the TESS mission are improving this. Stars with radiative envelopes have little mixing at their surface, and thus their surface abundances provide a sensitive test case for a variety of processes, including potentially star-planet…

2022 Astronomy and Astrophysics
Gaia 5
Removal of straylight from ExoMars NOMAD-UVIS observations
DOI: 10.1016/j.pss.2022.105432 Bibcode: 2022P&SS..21805432M

Vandaele, Ann Carine; Daerden, Frank; Ristic, Bojan +13 more

We present an in-flight straylight removal method for the Ultraviolet and Visible Spectrometer (UVIS) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument aboard the ExoMars Trace Gas Orbiter (TGO). The presence of a 'red-leak' straylight signal in the UVIS instrument was discovered post-launch in ground calibration measureme…

2022 Planetary and Space Science
ExoMars-16 5
Detection of Stellar-like Abundance Anomalies in the Slow Solar Wind
DOI: 10.3847/2041-8213/ac6878 Bibcode: 2022ApJ...930L..10B

Warren, Harry P.; Brooks, David H.; Baker, Deborah +2 more

The elemental composition of the Sun's hot atmosphere, the corona, shows a distinctive pattern that is different from the underlying surface or photosphere. Elements that are easy to ionize in the chromosphere are enhanced in abundance in the corona compared to their photospheric values. A similar pattern of behavior is often observed in the slow-…

2022 The Astrophysical Journal
SOHO 5