Search Publications

Galactic calibration of the tip of the red giant branch
DOI: 10.1017/pasa.2018.46 Bibcode: 2019PASA...36....1M

Clementini, Gisella; Da Costa, Gary; Mould, Jeremy

Indications from Gaia data release 2 are that the tip of the red giant branch (a population II standard candle related to the helium flash in low mass stars) is close to -4 in absolute I magnitude in the Cousins photometric system. Our sample is high-latitude southern stars from the thick disk and inner halo, and our result is consistent with long…

2019 Publications of the Astronomical Society of Australia
Gaia 16
Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances
DOI: 10.3847/1538-4357/ab02fc Bibcode: 2019ApJ...873...18Y

Yang, Wuming

Standard solar models (SSMs) constructed in accord with low metal abundances disagree with seismically inferred results. We constructed rotating solar models with low metal abundances that included enhanced settling and convection overshoot. In one of our rotating models, AGSSr2a, the convection overshoot allowed us to recover the radius of the ba…

2019 The Astrophysical Journal
SOHO 16
Formation of coronal rain triggered by impulsive heating associated with magnetic reconnection
DOI: 10.1051/0004-6361/201936253 Bibcode: 2019A&A...630A.123K

Kohutova, P.; Verwichte, E.; Froment, C.

Context. Coronal rain consists of cool plasma condensations formed in coronal loops as a result of thermal instability. The standard models of coronal rain formation assume that the heating is quasi-steady and localised at the coronal loop footpoints.
Aims: We present an observation of magnetic reconnection in the corona and the associated im…

2019 Astronomy and Astrophysics
IRIS 16
Angular momentum of z ∼ 1.5 galaxies and their local analogues with adaptive optics
DOI: 10.1093/mnras/stz750 Bibcode: 2019MNRAS.485.5700S

Glazebrook, Karl; Fisher, Deanne B.; Obreschkow, Danail +9 more

We present stellar specific angular momentum j* measurements of two z ∼ 1.5 galaxies in the KGES sample and 12 DYNAMO z ∼ 0.1 analogues of high-redshift galaxies. We combine natural seeing integral field spectroscopic data to trace line emission out to high multiples of effective radius re, with adaptive optics assisted Keck/…

2019 Monthly Notices of the Royal Astronomical Society
eHST 16
K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists
DOI: 10.3847/1538-3881/aafa70 Bibcode: 2019AJ....157...40F

Schlieder, Joshua E.; Howard, Andrew W.; Petigura, Erik A. +23 more

Observations from the Kepler and K2 missions have provided the astronomical community with unprecedented amounts of data to search for transiting exoplanets and other astrophysical phenomena. Here, we present K2-288, a low-mass binary system (M2.0 ± 1.0; M3.0 ± 1.0) hosting a small (R p = 1.9 R ), temperate (T eq

2019 The Astronomical Journal
Gaia 16
Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004-2017
DOI: 10.3847/1538-4365/ab3799 Bibcode: 2019ApJS..244...14N

Bézard, Bruno; Vinatier, Sandrine; Lellouch, Emmanuel +16 more

From 2004 to 2017, the Cassini spacecraft orbited Saturn, completing 127 close flybys of its largest moon, Titan. Cassini’s Composite Infrared Spectrometer (CIRS), one of 12 instruments carried on board, profiled Titan in the thermal infrared (7-1000 µm) throughout the entire 13 yr mission. CIRS observed on both targeted encounters (flybys) …

2019 The Astrophysical Journal Supplement Series
Cassini 16
XMM-Newton observations of PSR J0726-2612, a radio-loud XDINS
DOI: 10.1051/0004-6361/201935485 Bibcode: 2019A&A...627A..69R

Pintore, Fabio; Mereghetti, Sandro; Turolla, Roberto +4 more

We present the results of an XMM-Newton observation of the slowly rotating (P = 3.4 s), highly magnetized (B ≈ 3 × 1013 G) radio pulsar PSR J0726-2612. A previous X-ray observation with the Chandra satellite showed that some of the properties of PSR J0726-2612 are similar to those of the X-ray-dim isolated neutron stars (XDINSs), a smal…

2019 Astronomy and Astrophysics
XMM-Newton 16
Properties of the Umbral Filament Observed in Active Region NOAA 12529
DOI: 10.3847/1538-4357/ab2635 Bibcode: 2019ApJ...880...34G

Murabito, Mariarita; Guglielmino, Salvo L.; Romano, Paolo +2 more

Recent observations of the solar photosphere revealed the presence of elongated filamentary bright structures inside sunspot umbrae, called umbral filaments (UFs). These features differ in morphology, magnetic configuration, and evolution from light bridges (LBs) that are usually observed to intrude in sunspots. To characterize a UF observed in th…

2019 The Astrophysical Journal
Hinode IRIS 16
Fluorine Abundances in the Galactic Disk
DOI: 10.3847/1538-4357/ab45f1 Bibcode: 2019ApJ...885..139G

Cunha, Katia; Smith, Verne V.; Hayes, Christian R. +5 more

The chemical evolution of fluorine is investigated in a sample of Milky Way red giant stars that span a significant range in metallicity from [Fe/H] ∼ -1.3 to 0.0 dex. Fluorine abundances are derived from vibration-rotation lines of HF in high-resolution infrared spectra near 2.335 µm. The red giants are members of the thin and thick disk/ha…

2019 The Astrophysical Journal
Gaia 16
CPCS 2.0 — new automatic tool for time-domain astronomy
Bibcode: 2019CoSka..49..125Z

Rybicki, K.; Wyrzykowski, Ł.; Zieliński, P. +3 more

The Cambridge Photometric Calibration Server (CPCS) has been designed to respond to the need of automated rapid photometric data calibration and dissemination for transient events, primarily from Gaia space mission. The Calibration Server has been in operation since 2013 and has been used to calibrate around 50 000 observations of hundreds of tran…

2019 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 16