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HD 219134 Revisited: Planet d Transit Upper Limit and Planet f Transit Nondetection with ASTERIA and TESS
DOI: 10.3847/1538-3881/abcd3d Bibcode: 2021AJ....161..117S

Vanderburg, Andrew; Latham, David W.; Schlieder, Joshua E. +38 more

HD 219134 is a K3V dwarf star with six reported radial-velocity discovered planets. The two innermost planets b and c show transits, raising the possibility of this system to be the nearest (6.53 pc), brightest (V = 5.57) example of a star with a compact multiple transiting planet system. Ground-based searches for transits of planets beyond b and …

2021 The Astronomical Journal
Gaia 7
Reconstruction of Magnetospheric Storm Time Dynamics Using Cylindrical Basis Functions and Multi Mission Data Mining
DOI: 10.1029/2020JA028390 Bibcode: 2021JGRA..12628390T

Sitnov, M. I.; Tsyganenko, N. A.; Andreeva, V. A.

First results are presented of the modeling of magnetospheric storm events, based on: (i) a new method to represent the magnetic field by means of the so called cylindrical basis functions, (ii) the data mining approach by Sitnov et al. (2008); https://doi.org/10.1029/2007ja013003, and (iii) upgra…

2021 Journal of Geophysical Research (Space Physics)
Cluster 7
The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
DOI: 10.1017/pasa.2021.26 Bibcode: 2021PASA...38...33B

Pozzi, F.; Rodighiero, G.; Feltre, A. +21 more

In the black hole (BH)-galaxy co-evolution framework, most of the star formation (SF) and the BH accretion are expected to take place in highly obscured conditions. The large amount of gas and dust absorbs most of the UV-to-soft-X radiation and re-emits it at longer wavelengths, mostly in the IR. Thus, obscured active galactic nuclei (AGN) are ver…

2021 Publications of the Astronomical Society of Australia
Herschel 7
Constraining Progenitors of Observed Low-mass X-ray Binaries Using Convection and Rotation-Boosted Magnetic Braking
DOI: 10.3847/1538-4357/ac236c Bibcode: 2021ApJ...922..174V

Van, Kenny X.; Ivanova, Natalia

We present a new method for constraining the mass transfer evolution of low-mass X-ray binaries (LMXBs)-a reverse population synthesis technique. This is done using the detailed 1D stellar evolution code MESA (Modules for Experiments in Stellar Astrophysics) to evolve a high-resolution grid of binary systems spanning a comprehensive range of initi…

2021 The Astrophysical Journal
Gaia 7
Revisiting Newly Large Magellanic Cloud Age-gap Star Clusters
DOI: 10.3847/1538-3881/abe545 Bibcode: 2021AJ....161..199P

Piatti, Andrés E.

Recently, a noticeable number of new star clusters was identified in the outskirts of the Large Magellanic Cloud (LMC) populating the so-called star-cluster age gap, a space of time (∼4-12 Gyr) where the only known star cluster is up-to-date ESO 121-SC 03. We used Survey of the Magellanic Stellar History DR2 data sets, as well as those employed to…

2021 The Astronomical Journal
Gaia 7
Evolution of galaxy scaling relations in clusters at 0.5 < z < 1.5
DOI: 10.1051/0004-6361/201936456 Bibcode: 2021A&A...646A..53P

Böhm, A.; Dannerbauer, H.; Hoyos, C. +4 more


Aims: We present new gas kinematic observations with the OSIRIS instrument at the GTC for galaxies in the Cl1604 cluster system at z ∼ 0.9. These observations together with a collection of other cluster samples at different epochs analyzed by our group are used to study the evolution of the Tully-Fisher, velocity-size, and specific angular mo…

2021 Astronomy and Astrophysics
eHST 7
The precessing jets of classical nova YZ Reticuli
DOI: 10.1093/mnras/stab581 Bibcode: 2021MNRAS.503..704M

Blundell, Katherine M.; Lee, Steven; McLoughlin, Dominic +1 more

The classical nova YZ Reticuli was discovered in 2020 July. Shortly after this, we commenced a sustained, highly time-sampled coverage of its subsequent rapid evolution with time-resolved spectroscopy from the Global Jet Watch observatories. Its H-alpha complex exhibited qualitatively different spectral signatures in the following weeks and months…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 7
Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299
DOI: 10.3847/2041-8213/ac1945 Bibcode: 2021ApJ...918L..17M

Fukazawa, Yasushi; Gu, Liyi; Zhou, Ping +8 more

Hot atmospheres of massive galaxies are enriched with metals. Elemental abundances measured in the X-ray band have been used to study the chemical enrichment of supernova remnants, elliptical galaxies, groups, and clusters of galaxies. Here we measure the elemental abundances of the hot atmosphere of luminous infrared galaxy Arp 299 observed with …

2021 The Astrophysical Journal
XMM-Newton 7
The mid-infrared Leavitt law for classical Cepheids in the Magellanic Clouds
DOI: 10.1093/mnras/staa3186 Bibcode: 2021MNRAS.500..817C

Wuyts, Stijn; Scowcroft, Victoria; Chown, Abigail H.

The Cepheid Leavitt Law (LL), also known as the Period-Luminosity relation, is a crucial tool for assembling the cosmic distance ladder. By combining data from the OGLE-IV catalogue with mid-infrared photometry from the Spitzer Space Telescope, we have determined the 3.6 and 4.5 $\mu$m LLs for the Magellanic Clouds using ~5000 fundamental-mode cla…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 7
2MASX J00423991 + 3017515: an offset active galactic nucleus in an interacting system
DOI: 10.1093/mnras/stab576 Bibcode: 2021MNRAS.503.1688H

Reynolds, Christopher S.; Blecha, Laura; Smith, Krista Lynne +2 more

We present a spectroscopic and imaging study of an abnormal active galactic nucleus (AGN), 2MASX J00423991 + 3017515. This AGN is newly identified in the hard X-rays by the Swift BAT All-Sky survey and found in an edge-on disc galaxy interacting with a nearby companion. Here, we analyse the first optical spectra obtained for this system (taken in …

2021 Monthly Notices of the Royal Astronomical Society
eHST 7