Search Publications

A Late-type L Dwarf at 11 pc Hiding in the Galactic Plane Characterized Using Gaia DR2
DOI: 10.3847/1538-4357/aadd04 Bibcode: 2018ApJ...868...44F

Gonzales, Eileen C.; Burgasser, Adam J.; Marocco, Federico +4 more

We report on the characterization of a nearby (d={11.20}-0.08+0.09 pc) ultracool L dwarf (WISE J192512.78+070038.8; hereafter W1925) identified as a faint (G = 20.038 ± 0.009) object with high proper motion (219.834 ± 1.843 mas yr-1)in the Gaia Data Releases 1 and 2. A Palomar/TripleSpec near-infrared spectrum of W…

2018 The Astrophysical Journal
Gaia 17
Late Bloomer Galaxies: Growing Up in Cosmic Autumn
DOI: 10.3847/1538-4357/aaedbe Bibcode: 2018ApJ...869..152D

Kelson, Daniel D.; Dressler, Alan; Abramson, Louis E.

Late bloomers (LBs) are massive ({M}* > {10}10 {\text{}}{M}) galaxies at z < 1 that formed the majority of their stars within ∼2 Gyr of the epoch of observation. Our improved methodology for deriving star formation histories (SFHs) of galaxies at redshifts 0.45 < z < 0.75 from the Carnegie-Spitzer-IMA…

2018 The Astrophysical Journal
eHST 17
Density Fluctuations in a Polar Coronal Hole
DOI: 10.3847/1538-4357/aac0f3 Bibcode: 2018ApJ...860...34H

Hahn, Michael; D'Huys, Elke; Savin, Daniel Wolf

We have measured the root-mean-square (rms) amplitude of intensity fluctuations, ΔI, in plume and interplume regions of a polar coronal hole. These intensity fluctuations correspond to density fluctuations. Using data from the Sun Watcher using the Active Pixel System detector and Image Processing on the Project for Onboard Autonomy (Proba2), our …

2018 The Astrophysical Journal
PROBA-2 17
High Spectral Resolution SOFIA/EXES Observations of C2H2 toward Orion IRc2
DOI: 10.3847/1538-4357/aaab66 Bibcode: 2018ApJ...856....9R

Le Gal, Romane; Herbst, Eric; Acharyya, Kinsuk +8 more

We present high spectral resolution observations from 12.96 to 13.33 microns toward Orion IRc2 using the mid-infrared spectrograph, Echelon-Cross-Echelle Spectrograph (EXES), at Stratospheric Observatory for Infrared Astronomy (SOFIA). These observations probe the physical and chemical conditions of the Orion hot core, which is sampled by a bright…

2018 The Astrophysical Journal
ISO 17
Resolving the Inner Arcsecond of the RY Tau Jet with HST
DOI: 10.3847/1538-4357/aaab58 Bibcode: 2018ApJ...855..143S

Skinner, Stephen L.; Güdel, Manuel; Audard, Marc +1 more

Faint X-ray emission from hot plasma (T x > 106 K) has been detected extending outward a few arcseconds along the optically delineated jets of some classical T Tauri stars including RY Tau. The mechanism and location where the jets are heated to X-ray temperatures are unknown. We present high spatial resolution Hubble Sp…

2018 The Astrophysical Journal
eHST 17
A UV-to-NIR Study of Molecular Gas in the Dust Cavity around RY Lupi
DOI: 10.3847/1538-4357/aaaf65 Bibcode: 2018ApJ...855...98A

France, K.; Alcalá, J. M.; Williams, J. P. +10 more

We present a study of molecular gas in the inner disk (r< 20 {au}) around RY Lupi, with spectra from HST-COS, HST-STIS, and VLT-CRIRES. We model the radial distribution of flux from hot gas in a surface layer between r = 0.1-10 au, as traced by Lyα-pumped H2. The result shows H2 emission originating in a ring centered at ∼…

2018 The Astrophysical Journal
eHST 17
An Unexpected Detection of Bifurcated Blue Straggler Sequences in the Young Globular Cluster NGC 2173
DOI: 10.3847/1538-4357/aaad65 Bibcode: 2018ApJ...856...25L

Deng, Licai; de Grijs, Richard; Li, Chengyuan +2 more

The bifurcated patterns in the color-magnitude diagrams of blue straggler stars (BSSs) have attracted significant attention. This type of special (but rare) pattern of two distinct blue straggler sequences is commonly interpreted as evidence that cluster core-collapse-driven stellar collisions are an efficient formation mechanism. Here, we report …

2018 The Astrophysical Journal
eHST 17
Mapping Lyman Continuum Escape in Tololo 1247-232
DOI: 10.3847/1538-4357/aae372 Bibcode: 2018ApJ...867....2M

Jaskot, Anne E.; James, Bethan L.; Oey, M. S. +2 more

Low-redshift, spatially resolved Lyman continuum (LyC) emitters allow us to clarify the processes for LyC escape from these starburst galaxies. We use Hubble Space Telescope (HST) WFC3 and ACS imaging of the confirmed low-redshift LyC emitter Tol 1247-232 to study the ionization structure of the gas and its relation to the ionizing star clusters. …

2018 The Astrophysical Journal
eHST 17
Herschel PACS Observations of 4-10 Myr Old Classical T Tauri Stars in Orion OB1
DOI: 10.3847/1538-4357/aabf40 Bibcode: 2018ApJ...859....1M

Qi, Chunhua; Calvet, Nuria; Espaillat, Catherine C. +12 more

We present Herschel PACS observations of eight classical T Tauri Stars in the ∼7-10 Myr old OB1a and the ∼4-5 Myr old OB1b Orion subassociations. Detailed modeling of the broadband spectral energy distributions, particularly the strong silicate emission at 10 µm, shows that these objects are (pre-)transitional disks with some amount of small…

2018 The Astrophysical Journal
Herschel 17
Asteroseismology of the Double-mode High-amplitude δ Scuti Star VX Hydrae
DOI: 10.3847/1538-4357/aac9c5 Bibcode: 2018ApJ...861...96X

Fu, Jian-Ning; Su, Jie; Castro, A. +11 more

Bi-site time-series photometric and high-resolution spectroscopic observations were made for the double-mode high-amplitude δ Scuti star VX Hya. The fundamental frequency f 0 = 4.4763 c days-1, the first overtone f 1 = 5.7897 c days-1, and 23 harmonics and linear combinations of f 0 and f

2018 The Astrophysical Journal
Gaia 17