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The β Pictoris b Hill sphere transit campaign. I. Photometric limits to dust and rings
DOI: 10.1051/0004-6361/202040060 Bibcode: 2021A&A...648A..15K

Wang, L.; Lecavelier des Etangs, A.; Stee, P. +33 more


Aims: Photometric monitoring of β Pic in 1981 showed anomalous fluctuations of up to 4% over several days, consistent with foreground material transiting the stellar disk. The subsequent discovery of the gas giant planet β Pic b and the predicted transit of its Hill sphere to within a 0.1 au projected separation of the planet provided an oppo…

2021 Astronomy and Astrophysics
eHST 11
Stellar loci IV. red giant stars
DOI: 10.1088/1674-4527/21/12/319 Bibcode: 2021RAA....21..319Z

Yuan, Hai-Bo; Huang, Yang; Chen, Bing-Qiu +3 more

In the fourth paper of this series, we present the metallicity-dependent Sloan Digital Sky Survey (SDSS) stellar color loci of red giant stars, using a spectroscopic sample of red giants in the SDSS Stripe 82 region. The stars span a range of 0.55 - 1.2 mag in color g - i, -0.3 - -2.5 in metallicity [Fe/H], and have values of surface gravity log g…

2021 Research in Astronomy and Astrophysics
Gaia 11
Discovery of a Protocluster Core Associated with an Enormous Lya Nebula at z = 2.3
DOI: 10.3847/1538-4357/ac29c6 Bibcode: 2021ApJ...922..236L

Fan, Xiaohui; Cai, Zheng; Li, Qiong +10 more

The MAMMOTH-1 nebula at z = 2.317 is an enormous Lyα nebula (ELAN) extending to a ~440 kpc scale at the center of the extreme galaxy overdensity BOSS 1441. In this paper, we present observations of the CO(3 - 2) and 250 GHz dust-continuum emission from MAMMOTH-1 using the IRAM NOrthern Extended Millimeter Array. Our observations show that CO(3 - 2…

2021 The Astrophysical Journal
eHST 11
Radio evidence for a shock wave reflected by a coronal hole
DOI: 10.1051/0004-6361/202141387 Bibcode: 2021A&A...651L..14M

Bemporad, A.; Frassati, F.; Giordano, S. +4 more

We report the first unambiguous observational evidence in the radio range of the reflection of a coronal shock wave at the boundary of a coronal hole. The event occurred above an active region located at the northwest limb of the Sun and was characterized by an eruptive prominence and an extreme-ultraviolet wave steepening into a shock. The EUV ob…

2021 Astronomy and Astrophysics
PROBA-2 SOHO 11
A Spatially Resolved Survey of Distant Quasar Host Galaxies. II. Photoionization and Kinematics of the ISM
DOI: 10.3847/1538-4357/abddc1 Bibcode: 2021ApJ...910...44V

Armus, Lee; Larkin, James E.; Wright, Shelley A. +6 more

We present detailed observations of photoionization conditions and galaxy kinematics in 11 z = 1.39-2.59 radio-loud quasar host galaxies. Data were taken with the OSIRIS integral field spectrograph and the adaptive optics system at the W. M. Keck Observatory that targeted nebular emission lines (Hβ, [O III], Hα, [N II]) redshifted into the near-in…

2021 The Astrophysical Journal
eHST 11
The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.6 and 1.2
DOI: 10.1093/mnras/stab1638 Bibcode: 2021MNRAS.506..473P

McHardy, I.; Page, M. J.; Symeonidis, M. +11 more

We use ultraviolet (UV) imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 arcmin2 in the UVW1 band (λeff = 2910 Å) to measure rest-frame UV 1500-Å luminosity functions of galaxies with redshifts z between 0.6 and 1.2. The XMM-OM data are supplemented by a large body of optical and infrared ima…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11
A stellar census in globular clusters with MUSE. A new perspective on the multiple main sequences of ω Centauri
DOI: 10.1051/0004-6361/202141791 Bibcode: 2021A&A...653L...8L

Dreizler, S.; Latour, M.; Brinchmann, J. +3 more

Context. ω Cen is a rare example of a globular cluster where the iron abundance of the stars spans more than one order of magnitude. Many spectroscopic investigations of its red-giant and sub-giant branches have revealed multiple peaks in the iron abundance distribution. The metallicity distribution of main sequence (MS) stars is not well characte…

2021 Astronomy and Astrophysics
eHST 11
Years-delayed X-Ray Afterglows of TDEs Originated from Wind-Torus Interactions
DOI: 10.3847/1538-4357/abd475 Bibcode: 2021ApJ...908..197M

Wang, Wei; Shu, Xinwen; Jiang, Ning +8 more

Tidal disruption events (TDEs) occurring in active galactic nuclei (AGNs) are a special class of sources with outstanding scientific significance. TDEs can generate ultrafast winds, which should almost inevitably collide with the preexisting AGN dusty tori. We perform analytical calculations and simulations on the wind-torus interactions and find …

2021 The Astrophysical Journal
XMM-Newton 11
Mid-infrared reflectance spectroscopy of synthetic glass analogs for Mercury surface studies
DOI: 10.1016/j.icarus.2021.114363 Bibcode: 2021Icar..36114363M

Helbert, Joern; Hiesinger, Harald; Weber, Iris +14 more

We have synthesized and analyzed by mid-infrared reflectance spectroscopy silicate glasses that are representative for the glasses on the surface of Mercury. The glass compositions are based on high-pressure laboratory experiments and the resulting compositions of the glass phase. The spectra are of interest for investigating the surface of Mercur…

2021 Icarus
BepiColombo 11
NGTS 15b, 16b, 17b, and 18b: four hot Jupiters from the Next-Generation Transit Survey
DOI: 10.1093/mnras/stab815 Bibcode: 2021MNRAS.504.6018T

Wheatley, Peter J.; Bayliss, Daniel; Worters, Hannah L. +36 more

We report the discovery of four new hot Jupiters with the Next-Generation Transit Survey (NGTS). NGTS-15b, NGTS-16b, NGTS-17b, and NGTS-18b are short-period (P < 5 d) planets orbiting G-type main-sequence stars, with radii and masses between 1.10 and 1.30RJ and 0.41 and 0.76MJ, respectively. By considering the host star lu…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 11