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High-resolution ALMA and HST images of q1 Eri: an asymmetric debris disc with an eccentric Jupiter
DOI: 10.1093/mnras/stab1678 Bibcode: 2021MNRAS.506.1978L

Krist, J.; Stapelfeldt, K.; Kral, Q. +10 more

We present Atacama Large Millimetre/sub-Millimetre Array (ALMA) 1.3 and 0.86 mm observations of the nearby (17.34 pc) F9V star q1 Eri (HD 10647, HR 506). This system, with age ~1.4 Gyr, hosts a ~2 au radial velocity planet and a debris disc with the highest fractional luminosity of the closest 300 FGK type stars. The ALMA images, with resolution ~…

2021 Monthly Notices of the Royal Astronomical Society
AKARI Gaia eHST 24
Correction to the Photometric Colors of the Gaia Data Release 2 with the Stellar Color Regression Method
DOI: 10.3847/1538-4357/abdbac Bibcode: 2021ApJ...909...48N

Niu, Zexi; Liu, Jifeng; Yuan, Haibo

The second Gaia data release (DR2) delivers accurate and homogeneous photometry data of the whole sky of an exquisite quality, reaching down to the unprecedented millimagnitude (mmag) level for the G, GRP, and GBP passbands. However, the presence of magnitude-dependent systematic effects at the 10 mmag level limits its power …

2021 The Astrophysical Journal
Gaia 24
Tidal tails in the disintegrating open cluster NGC 752
DOI: 10.1093/mnras/stab1404 Bibcode: 2021MNRAS.505.1607B

Vaidya, Kaushar; Rao, Khushboo K.; Agarwal, Manan +1 more

We utilize the robust membership determination algorithm, ML-MOC, on the precise astrometric and deep photometric data from Gaia Early Data Release 3 within a region of radius 5° around the centre of the intermediate-age Galactic open cluster NGC 752 to identify its member stars. We report the discovery of the tidal tails of NGC 752, extending out…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
Evidence of a Clear Atmosphere for WASP-62b: The Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone
DOI: 10.3847/2041-8213/abd18e Bibcode: 2021ApJ...906L..10A

Nikolov, Nikolay; Mikal-Evans, Thomas; Sing, David K. +12 more

Exoplanets with cloud-free, haze-free atmospheres at the pressures probed by transmission spectroscopy represent a valuable opportunity for detailed atmospheric characterization and precise chemical abundance constraints. We present the first optical to infrared (0.3-5 µm) transmission spectrum of the hot Jupiter WASP-62b, measured with Hubb…

2021 The Astrophysical Journal
XMM-Newton 24
WISDOM project - VII. Molecular gas measurement of the supermassive black hole mass in the elliptical galaxy NGC 7052
DOI: 10.1093/mnras/stab791 Bibcode: 2021MNRAS.503.5984S

Williams, Thomas G.; Sarzi, Marc; Cappellari, Michele +7 more

Supermassive black hole (SMBH) masses can be measured by resolving the dynamical influences of the SMBHs on tracers of the central potentials. Modern long-baseline interferometers have enabled the use of molecular gas as such a tracer. We present here Atacama Large Millimeter/submillimeter Array observations of the elliptical galaxy NGC 7052 at 0.…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
Tracing PAH Size in Prominent Nearby Mid-Infrared Environments
DOI: 10.3847/1538-4357/ac02c6 Bibcode: 2021ApJ...918....8K

Tielens, A. G. G. M.; Peeters, E.; Vacca, W. D. +2 more

We present observations from the First Light Infrared TEst CAMera (FLITECAM) on board the Stratospheric Observatory for Infrared Astronomy, the Spitzer Infrared Array Camera (IRAC), and the Spitzer Infrared Spectrograph SH mode in three well-known photodissociation regions, the reflection nebulae (RNe) NGC 7023 and NGC 2023 and to the southeast of…

2021 The Astrophysical Journal
AKARI Gaia ISO 23
Correction to the Photometric Magnitudes of the Gaia Early Data Release 3
DOI: 10.3847/2041-8213/abdbae Bibcode: 2021ApJ...908L..24Y

Huang, Yang; Niu, Zexi; Yuan, Haibo +4 more

In this Letter, we have carried out an independent validation of the Gaia Early Data Release 3 (EDR3) photometry using approximately 10,000 Landolt standard stars from Clem & Landolt (2013). Using a machine-learning technique, the UBVRI magnitudes are converted into the Gaia magnitudes and colors and then compared to those in the EDR3, with th…

2021 The Astrophysical Journal
Gaia 23
A method for finding anomalous astronomical light curves and their analogues
DOI: 10.1093/mnras/stab2588 Bibcode: 2021MNRAS.508.5734M

Graham, Matthew J.; Giles, Daniel; Mahabal, Ashish A. +4 more

Our understanding of the Universe has profited from deliberate targeted studies of known phenomena, as well as from serendipitous unexpected discoveries, such as the discovery of a complex variability pattern in the direction of KIC 8462852 (Boyajian's star). Upcoming surveys such as the Vera C. Rubin Observatory Legacy Survey of Space and Time wi…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 23
A proto-helium white dwarf stripped by a substellar companion via common-envelope ejection. Uncovering the true nature of a candidate hypervelocity B-type star
DOI: 10.1051/0004-6361/202038757 Bibcode: 2021A&A...650A.102I

Geier, S.; Heber, U.; Irrgang, A. +3 more

In the past, SDSS J160429.12+100002.2 wass spectroscopically classified as a blue horizontal branch (BHB) star. Assuming a luminosity that is characteristic of BHB stars, the object's radial velocity and proper motions from Gaia Early Data Release 3 would imply that its Galactic rest-frame velocity exceeds its local escape velocity. Consequently, …

2021 Astronomy and Astrophysics
Gaia 23
The centres of M83 and the Milky Way: opposite extremes of a common star formation cycle
DOI: 10.1093/mnras/stab1527 Bibcode: 2021MNRAS.505.4310C

Henshaw, Jonathan D.; Kruijssen, J. M. Diederik; Longmore, Steven N. +8 more

In the centres of the Milky Way and M83, the global environmental properties thought to control star formation are very similar. However, M83's nuclear star formation rate (SFR), as estimated by synchrotron and H α emission, is an order of magnitude higher than the Milky Way's. To understand the origin of this difference we use ALMA observations o…

2021 Monthly Notices of the Royal Astronomical Society
eHST 23