Search Publications

Observations of Magnetic Fields Surrounding LkHα 101 Taken by the BISTRO Survey with JCMT-POL-2
DOI: 10.3847/1538-4357/abd0fc Bibcode: 2021ApJ...908...10N

Zhang, Yapeng; Pattle, Kate; Ward-Thompson, Derek +146 more

We report the first high spatial resolution measurement of magnetic fields surrounding LkHα 101, part of the Auriga-California molecular cloud. The observations were taken with the POL-2 polarimeter on the James Clerk Maxwell Telescope within the framework of the B-fields In Star-forming Region Observations (BISTRO) survey. Observed polarization o…

2021 The Astrophysical Journal
Gaia Herschel 29
The Atacama Cosmology Telescope: Probing the baryon content of SDSS DR15 galaxies with the thermal and kinematic Sunyaev-Zel'dovich effects
DOI: 10.1103/PhysRevD.104.043503 Bibcode: 2021PhRvD.104d3503V

Bond, J. R.; Calabrese, E.; Huffenberger, K. M. +51 more

We present measurements of the average thermal Sunyaev Zel'dovich (tSZ) effect from optically selected galaxy groups and clusters at high signal-to-noise (up to 12 σ ) and estimate their baryon content within a 2.1' radius aperture. Sources from the Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey DR15 catalog overlap wi…

2021 Physical Review D
Herschel 29
A preserved high-z compact progenitor in the heart of NGC 3311 revealed with MUSE 2D stellar population analysis
DOI: 10.1051/0004-6361/202039809 Bibcode: 2021A&A...649A..93B

Hilker, M.; Richtler, T.; Coccato, L. +3 more

Context. Massive early-type galaxies are believed to be the end result of an extended mass accretion history. The stars formed in situ very early on in the initial phase of the mass assembly might have originated from an extremely intense and rapid burst of star formation. These stars may still be found within the cores of such galaxies at z = 0, …

2021 Astronomy and Astrophysics
eHST 29
Stars and gas in the most metal-poor galaxies - I. COS and MUSE observations of SBS 0335-052E
DOI: 10.1093/mnras/staa3365 Bibcode: 2021MNRAS.500.2908W

Feltre, Anna; Charlot, Stéphane; Chevallard, Jacopo +5 more

Among the nearest most metal-poor starburst-dwarf galaxies known, SBS 0335-052E is the most luminous in integrated nebular He II λ4686 emission. This makes it a unique target to test spectral synthesis models and spectral interpretation tools of the kind that will be used to interpret future rest-frame UV observations of primeval galaxies. Previou…

2021 Monthly Notices of the Royal Astronomical Society
eHST 29
The source of the major solar energetic particle events from super active region 11944
DOI: 10.1126/sciadv.abf0068 Bibcode: 2021SciA....7...68B

Brooks, David H.; Yardley, Stephanie L.

Shock waves associated with fast coronal mass ejections (CMEs) accelerate solar energetic particles (SEPs) in the long duration, gradual events that pose hazards to crewed spaceflight and near-Earth technological assets, but the source of the CME shock-accelerated plasma is still debated. Here, we use multi-messenger observations from the Heliophy…

2021 Science Advances
Hinode 29
3D MHD astrospheres: applications to IRC-10414 and Betelgeuse
DOI: 10.1093/mnras/stab2026 Bibcode: 2021MNRAS.506.5170M

Meyer, D. M. -A.; Mignone, A.; Petrov, M. +3 more

A significative fraction of all massive stars in the Milky Way move supersonically through their local interstellar medium (ISM), producing bow shock nebulae by wind-ISM interaction. The stability of these observed astrospheres around cool massive stars challenges precedent 2D (magneto-)hydrodynamical (MHD) simulations of their surroundings. We pr…

2021 Monthly Notices of the Royal Astronomical Society
Herschel 29
The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics
DOI: 10.1051/0004-6361/202141374 Bibcode: 2021A&A...655A.105S

Sollerman, J.; Jerkstrand, A.; Filippenko, A. V. +25 more

We present the discovery and extensive follow-up observations of SN 2020jfo, a Type IIP supernova (SN) in the nearby (14.5 Mpc) galaxy M 61. Optical light curves (LCs) and spectra from the Zwicky Transient Facility (ZTF), complemented with data from Swift/UVOT and near-infrared photometry is presented. These were used to model the 350-day duration…

2021 Astronomy and Astrophysics
eHST 29
The ρ Ophiuchi region revisited with Gaia EDR3. Two young populations, new members, and old impostors
DOI: 10.1051/0004-6361/202140438 Bibcode: 2021A&A...652A...2G

Meingast, Stefan; Alves, João; Lombardi, Marco +10 more

Context. Young and embedded stellar populations are important probes of the star formation process. Their properties and the environments they create have the potential to affect the formation of new planets. Paradoxically, we have a better census of nearby embedded young populations than of the slightly more evolved optically visible young popula…

2021 Astronomy and Astrophysics
Gaia Herschel 29
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
DOI: 10.3847/1538-4357/ac2578 Bibcode: 2021ApJ...922..114S

Pérez-González, Pablo G.; Koekemoer, Anton M.; Smail, Ian +22 more

We present a Spitzer/IRAC survey of H-faint (H 160 ≳ 26.4, < 5σ) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of ~648 arcmin2 (effectively ~221 arcmin2 in the source plane), we have securely discovered 53 sources in the IRAC Channel-2 band (CH2, 4.5 µm; median CH2 = 22.46 ±…

2021 The Astrophysical Journal
Gaia Herschel eHST 29
Massive stars in the Small Magellanic Cloud. Evolution, rotation, and surface abundances
DOI: 10.1051/0004-6361/202039890 Bibcode: 2021A&A...647A.134B

Bouret, J. -C.; Martins, F.; Hillier, D. J. +5 more

Context. The evolution of massive stars depends on several physical processes and parameters. Metallicity and rotation are among the most important, but their quantitative effects are not well understood.
Aims: To complement our earlier study on main-sequence stars, we study the evolutionary and physical properties of evolved O stars in the S…

2021 Astronomy and Astrophysics
eHST 29