Search Publications

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
Variable oxygen emission from the accretion disk of Mrk 110
DOI: 10.1051/0004-6361/202140953 Bibcode: 2021A&A...649L...3R

Grosso, N.; Porquet, D.; Reeves, J. N. +2 more

Six XMM-Newton observations of the bright narrow line Seyfert 1, Mrk 110, from 2004-2020, are presented. The analysis of the grating spectra from the Reflection Grating Spectrometer (RGS) reveals a broad component of the He-like Oxygen (O VII) line, with a full width at half maximum of 15 900 ± 1800 km s−1 measured in the mean spectrum.…

2021 Astronomy and Astrophysics
XMM-Newton 6
V680 Mon - a young mercury-manganese star in an eclipsing heartbeat system
DOI: 10.1093/mnras/stab1059 Bibcode: 2021MNRAS.504.3749P

Vaňko, Martin; Paunzen, Ernst; Hümmerich, Stefan +3 more

Chemically peculiar stars in eclipsing binary systems are rare objects that allow the derivation of fundamental stellar parameters and important information on evolutionary status and the origin of the observed chemical peculiarities. Here we present an investigation of the known eclipsing binary system BD+09 1467 = V680 Mon. Using spectra from th…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 6
A deep XMM-Newton observation of the X-Persei-like binary system CXOU J225355.1+624336
DOI: 10.1051/0004-6361/202140760 Bibcode: 2021A&A...649A.118L

Sidoli, L.; Esposito, P.; La Palombara, N. +2 more

We report on the follow-up XMM-Newton observation of the persistent X-ray pulsar CXOU J225355.1+624336, which was discovered with the CATS@BAR project on archival Chandra data. The source was detected at fX(0.5−10 keV) = 3.4 × 10−12 erg cm−2 s−1, a flux level that is fully consistent with previous observ…

2021 Astronomy and Astrophysics
Gaia INTEGRAL XMM-Newton 6
Point spread function reconstruction of adaptive-optics imaging: meeting the astrometric requirements for time-delay cosmography
DOI: 10.1093/mnras/stab2587 Bibcode: 2021MNRAS.508..755C

Treu, Tommaso; Fassnacht, Christopher D.; Chen, Geoff C. -F. +3 more

Astrometric precision and knowledge of the point spread function are key ingredients for a wide range of astrophysical studies including time-delay cosmography in which strongly lensed quasar systems are used to determine the Hubble constant and other cosmological parameters. Astrometric uncertainty on the positions of the multiply-imaged point so…

2021 Monthly Notices of the Royal Astronomical Society
eHST 6
Magnetotail Processes
DOI: 10.1002/9781119815624.ch17 Bibcode: 2021GMS...259..245B

Khotyaintsev, Yuri; Runov, Andrei; Birn, Joachim

2021 Magnetospheres in the Solar System
Cluster 6
A Deep Census of Outlying Star Formation in the M101 Group
DOI: 10.3847/1538-4357/ac0055 Bibcode: 2021ApJ...915...57G

Mihos, J. Christopher; Harding, Paul; Watkins, Aaron E. +1 more

We present deep, narrowband imaging of the nearby spiral galaxy M101 and its group environment to search for star-forming dwarf galaxies and outlying H II regions. Using the Burrell Schmidt telescope, we target the brightest emission lines of star-forming regions, Hα, Hβ, and [O III], to detect potential outlying star-forming regions. Our survey c…

2021 The Astrophysical Journal
Gaia 6