Search Publications

Observation of bi-directional jets in a prominence
DOI: 10.1051/0004-6361/201935774 Bibcode: 2021A&A...651A..60H

Polito, V.; Hillier, A.

Quiescent prominences host a large range of flows, many driven by buoyancy, which lead to velocity shear. The presence of these shear flows could bend and stretch the magnetic field resulting in the formation of current sheets which can lead to magnetic reconnection. Though this has been hypothesised to occur in prominences, with some observations…

2021 Astronomy and Astrophysics
IRIS 6
Spectroscopic Monitoring of the Candidate Tidal Disruption Event in F01004-2237
DOI: 10.3847/1538-4357/abe049 Bibcode: 2021ApJ...909..159C

Jonker, Peter G.; Cannizzaro, Giacomo; Mata-Sánchez, D.

We present results of spectroscopic monitoring observations of the ultraluminous infrared galaxy F01004-2237. This galaxy was observed to undergo changes in its optical spectrum, detected by comparing a spectrum from 2015 with one from 2000. These changes were coincident with photometric brightening. The main changes detected in the optical spectr…

2021 The Astrophysical Journal
eHST 6
The Fundamental Plane of Massive Quiescent Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/abce66 Bibcode: 2021ApJ...908..135S

Conselice, Christopher J.; Gallazzi, Anna; Zibetti, Stefano +11 more

We examine the Fundamental Plane (FP) and mass-to-light ratio (M/L) scaling relations using the largest sample of massive quiescent galaxies at 1.5 < z < 2.5 to date. The FP (re, σe, Ie) is established using 19 UVJ quiescent galaxies from COSMOS with Hubble Space Telescope HF160W rest-frame optical…

2021 The Astrophysical Journal
eHST 6
Are we observing an NSC in course of formation in the NGC 4654 galaxy?
DOI: 10.1093/mnras/stab458 Bibcode: 2021MNRAS.503..594S

Mastrobuono-Battisti, A.; Georgiev, I. Y.; Capuzzo-Dolcetta, R. +2 more

We use direct N-body simulations to explore some possible scenarios for the future evolution of two massive clusters observed towards the centre of NGC 4654, a spiral galaxy with mass similar to that of the Milky Way. Using archival HST data, we obtain the photometric masses of the two clusters, M = 3 × 105 M and M = 1.7 × 1…

2021 Monthly Notices of the Royal Astronomical Society
eHST 6
Low-frequency Waves due to Newborn Interstellar Pickup He+ Observed by the Ulysses Spacecraft
DOI: 10.3847/1538-4357/ac2eb3 Bibcode: 2021ApJ...923..185M

Isenberg, Philip A.; Schwadron, Nathan A.; Murphy, Neil +8 more

We have surveyed magnetic field data from the Ulysses spacecraft and found examples of magnetic waves with the expected characteristics that point to excitation by newborn pickup He+. With interstellar neutrals as the likely source for the pickup ions, we have modeled the ion production rates and used them to produce wave excitation rat…

2021 The Astrophysical Journal
Ulysses 6
Seeking Echoes of Circumstellar Disks in Kepler Light Curves
DOI: 10.3847/1538-3881/ac05be Bibcode: 2021AJ....162...98B

Kenyon, Scott J.; Bromley, Benjamin C.; Leonard, Austin +3 more

Light echoes of flares on active stars offer the opportunity for direct detection of circumstellar dust. We revisit the problem of identifying faint echoes in postflare light curves, focusing on debris disks from ongoing planet formation. Starting with simulations, we develop an algorithm for estimating the radial extent and total mass from disk e…

2021 The Astronomical Journal
Gaia 6
Low surface brightness galaxies in z > 1 galaxy clusters: HST approaching the progenitors of local ultra diffuse galaxies
DOI: 10.1051/0004-6361/202040097 Bibcode: 2021A&A...646L..12B

Muzzin, Adam; Brammer, Gabriel; van der Burg, Remco F. J. +2 more

Ultra diffuse galaxies (UDGs) are a type of large low surface brightness (LSB) galaxies with particularly large effective radii (reff > 1.5 kpc) that are now routinely studied in the Local (z < 0.1) Universe. While they are found to be abundant in clusters, groups, and in the field, their formation mechanisms remain elusive and co…

2021 Astronomy and Astrophysics
Gaia eHST 6
Photospheric downflows observed with SDO/HMI, HINODE, and an MHD simulation
DOI: 10.1051/0004-6361/202040172 Bibcode: 2021A&A...647A.178R

Malherbe, J. M.; Roudier, T.; Ballot, J. +3 more

Downflows on the solar surface are suspected to play a major role in the dynamics of the convection zone, at least in its outer part. We investigate the existence of the long-lasting downflows whose effects influence the interior of the Sun but also the outer layers. We study the sets of Dopplergrams and magnetograms observed with Solar Dynamics O…

2021 Astronomy and Astrophysics
Hinode 6
Stellar, Gas, and Dust Emission of Star-forming Galaxies out to z ∼ 2
DOI: 10.3847/1538-4357/abf1e5 Bibcode: 2021ApJ...913...34N

Gronwall, Caryl; Ciardullo, Robin; Bowman, William P. +1 more

While dust is a major player in galaxy evolution, its relationship with gas and stellar radiation in the early universe is still not well understood. We combine 3D-Hubble Space Telescope emission-line fluxes with far-UV through far-IR photometry in a sample of 669 emission-line galaxies (ELGs) between 1.2 < z < 1.9 and use the MCSED spectral…

2021 The Astrophysical Journal
Herschel eHST 6
Multi-Point Observation of Hiss Emerging From Lightning Whistlers
DOI: 10.1029/2021JA029524 Bibcode: 2021JGRA..12629524S

Gurnett, Donald A.; Pickett, Jolene S.; Santolík, Ondřej +1 more

We analyze continuous multi-point measurements of electromagnetic field waveforms onboard the Cluster spacecraft in order to contribute to the discussion on sources of plasmaspheric hiss, known as a shaping agent for the Earth radiation belts. In our case study we aim at finding sources of hiss observed close to the geomagnetic equator in the oute…

2021 Journal of Geophysical Research (Space Physics)
Cluster 6