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The Habitable Zone Planet Finder Reveals a High Mass and Low Obliquity for the Young Neptune K2-25b
DOI: 10.3847/1538-3881/abb13a Bibcode: 2020AJ....160..192S

Mahadevan, Suvrath; Terrien, Ryan; Wisniewski, John +27 more

Using radial velocity data from the Habitable Zone Planet Finder, we have measured the mass of the Neptune-sized planet K2-25b, as well as the obliquity of its M4.5 dwarf host star in the 600-800 Myr Hyades cluster. This is one of the youngest planetary systems for which both of these quantities have been measured and one of the very few M dwarfs …

2020 The Astronomical Journal
Gaia 60
Large-scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
DOI: 10.3847/1538-4357/ab61fd Bibcode: 2020ApJ...890....7C

Papovich, Casey; Ferguson, Henry C.; Giavalisco, Mauro +14 more

We present a robust method, weighted von Mises kernel density estimation, along with boundary correction to reconstruct the underlying number density field of galaxies. We apply this method to galaxies brighter than Hubble Space Telescope $/{\rm{F}}160{\rm{w}}\leqslant 26$ AB mag in the redshift range 0.4 ≤ z ≤ 5 in the five CANDELS fields (GOODS-…

2020 The Astrophysical Journal
eHST 60
Temperatures and Metallicities of M Dwarfs in the APOGEE Survey
DOI: 10.3847/1538-4357/ab7004 Bibcode: 2020ApJ...892...31B

Hogg, David W.; Mann, Andrew W.; Burgasser, Adam +1 more

M dwarfs have enormous potential for our understanding of structure and formation on both Galactic and exoplanetary scales through their properties and compositions. However, current atmosphere models have limited ability to reproduce spectral features in stars at the coolest temperatures (Teff < 4200 K) and to fully exploit the info…

2020 The Astrophysical Journal
Gaia 60
Carbon star formation as seen through the non-monotonic initial-final mass relation
DOI: 10.1038/s41550-020-1132-1 Bibcode: 2020NatAs...4.1102M

Ramirez-Ruiz, Enrico; Girardi, Léo; Cheng, Sihao +13 more

The initial-final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR across astrophysics is universally acknowledged, not all of its fine details have yet been resolved. A new analysis of a few carbon-oxygen white dwarfs in old open clusters of the Milky Way led…

2020 Nature Astronomy
Gaia 60
Infrared detection of aliphatic organics on a cometary nucleus
DOI: 10.1038/s41550-019-0992-8 Bibcode: 2020NatAs...4..500R

Bellucci, G.; Carlson, R. W.; Fornasier, S. +28 more

The European Space Agency's Rosetta mission1 has acquired unprecedented measurements of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko (hereafter, 67P), the composition of which, as determined by in situ and remote-sensing instruments, including the VIRTIS instrument2, seems to be an assemblage of ices, mineral…

2020 Nature Astronomy
Rosetta 60
Hints on the origins of particle traps in protoplanetary disks given by the Mdust - M relation
DOI: 10.1051/0004-6361/201937003 Bibcode: 2020A&A...635A.105P

Pascucci, Ilaria; Pinilla, Paola; Marino, Sebastian

Context. Demographic surveys of protoplanetary disks, carried out mainly with the Atacama Large Millimeter/submillimete Array, have provided access to a large range of disk dust masses (Mdust) around stars with different stellar types and in different star-forming regions. These surveys found a power-law relation between Mdust

2020 Astronomy and Astrophysics
Gaia 59
Ram pressure stripping candidates in the coma cluster: evidence for enhanced star formation
DOI: 10.1093/mnras/staa1213 Bibcode: 2020MNRAS.495..554R

Parker, Laura C.; Roberts, Ian D.

The Coma cluster is the nearest massive (M ≳ 1015 M⊙) galaxy cluster, making it an excellent laboratory to probe the influence of the cluster environment on galaxy star formation. Here, we present a sample of 41 galaxies with disturbed morphologies consistent with ram pressure stripping. These galaxies are identified visually using high…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 59
Exploring Solar Wind Origins and Connecting Plasma Flows from the Parker Solar Probe to 1 au: Nonspherical Source Surface and Alfvénic Fluctuations
DOI: 10.3847/1538-4365/ab61f4 Bibcode: 2020ApJS..246...54P

D'Amicis, Raffaella; Réville, Victor; Velli, Marco +18 more

The magnetic field measurements of the FIELDS instrument on the Parker Solar Probe (PSP) have shown intensities, throughout its first solar encounter, that require a very low source surface (SS) height ( ${R}_{\mathrm{SS}}\leqslant 1.8\,{R}_{\odot }$ ) to be reconciled with magnetic field measurements at the Sun via potential field extrapolation (…

2020 The Astrophysical Journal Supplement Series
SOHO 59
The First Ultracompact Roche Lobe-Filling Hot Subdwarf Binary
DOI: 10.3847/1538-4357/ab72ff Bibcode: 2020ApJ...891...45K

Duev, Dmitry A.; Riddle, Reed; Szkody, Paula +29 more

We report the discovery of the first short-period binary in which a hot subdwarf star (sdOB) filled its Roche lobe and started mass transfer to its companion. The object was discovered as part of a dedicated high-cadence survey of the Galactic plane named the Zwicky Transient Facility and exhibits a period of P = 39.3401(1) minutes, making it the …

2020 The Astrophysical Journal
Gaia 59
How many components? Quantifying the complexity of the metallicity distribution in the Milky Way bulge with APOGEE
DOI: 10.1093/mnras/staa2807 Bibcode: 2020MNRAS.499.1037R

Monachesi, Antonela; Cohen, Roger E.; Cunha, Katia +16 more

We use data of ∼13-=000 stars from the Sloan Digital Sky Survey/Apache Point Observatory Galactic Evolution Experiment survey to study the shape of the bulge metallicity distribution function (MDF) within the region |ℓ| ≤ 11° and |b| ≤ 13°, and spatially constrained to RGC ≤ 3.5 kpc. We apply Gaussian mixture modelling and non-negative …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 59