2MASS J035523.37+113343.7: A YOUNG, DUSTY, NEARBY, ISOLATED BROWN DWARF RESEMBLING A GIANT EXOPLANET [0.03%]
2MASS J035523.37+113343.7：一个年轻、尘土飞扬、附近的孤立的褐矮星，类似于一颗巨行星 exoplanet)
Jacqueline K Faherty,Emily L Rice,Kelle L Cruz et al.
Jacqueline K Faherty et al.
We present parallax and proper motion measurements, near-infrared spectra, and WISE photometry for the low surface gravity L5γ dwarf 2MASSJ035523.37+113343.7 (2M0355). We use these data to evaluate photometric, spectral, and kinematic sign...
DISCOVERY OF TWO VERY WIDE BINARIES WITH ULTRACOOL COMPANIONS AND A NEW BROWN DWARF AT THE L/T TRANSITION [0.03%]
两颗拥有超冷伴星的宽轨道双星及一颗L/T界线附近的新褐矮星的发现
Koraljka Mužić,Jacqueline Radigan,Ray Jayawardhana et al.
Koraljka Mužić et al.
We present the discovery and spectroscopic follow-up of a nearby late-type L dwarf (2M0614+3950), and two extremely wide very-low-mass binary systems (2M0525-7425AB and 2M1348-1344AB), resulting from our search for common proper motion pair...
A New, Long-Lived, Jupiter Mesoscale Wave Observed at Visible Wavelengths [0.03%]
在可见光波长观测到的一种新的长期存在的木星中尺度波
Amy A Simon,Ricardo Hueso,Peio Iñurrigarro et al.
Amy A Simon et al.
Small-scale waves were observed along the boundary between Jupiter's North Equatorial Belt and North Tropical Zone, ~16.5° N planetographic latitude in Hubble Space Telescope data in 2012 and throughout 2015 to 2018, observable at all wave...
Jupiter's Mesoscale Waves Observed at 5 μ m by Ground-based Observations and Juno JIRAM [0.03%]
地面观测和朱诺号(Juno)的JIRAM仪在5μm波长下观测到的木星中尺度波动现象
Leigh N Fletcher,H Melin,A Adriani et al.
Leigh N Fletcher et al.
We characterize the origin and evolution of a mesoscale wave pattern in Jupiter's North Equatorial Belt (NEB), detected for the first time at 5 μm using a 2016-17 campaign of "lucky imaging" from the VISIR instrument on the Very Large Tele...
David Gordon,Christopher Jacobs,Anthony Beasley et al.
David Gordon et al.
Six very successful VLBA calibrator survey campaigns were run between 1994 and 2007 to build up a large list of compact radio sources with positions precise enough for use as VLBI phase reference calibrators. We report on the results of a s...
Spectroscopic Characterization of Key Aromatic Molecules: A Route toward The Origin of Life [0.03%]
关键芳香族化合物的光谱表征：通向生命起源的道路
Cristina Puzzarini,Alberto Baiardi,Julien Bloino et al.
Cristina Puzzarini et al.
To gain information on the abiotic synthesis of the building blocks of life from simple molecules, and their subsequent chemical evolution to biological systems, the starting point is the identification of target species in Titan-like plane...
FUSE Spectroscopy of the Accreting Hot Components in Symbiotic Variables [0.03%]
共生变星中吸积的热组件的FUSE光谱学研究
Edward M Sion,Patrick Godon,Joanna Mikolajewska et al.
Edward M Sion et al.
We have conducted a spectroscopic analysis of the far ultraviolet archival spectra of four symbiotic variables, EG And, AE Ara, CQ Dra and RW Hya. RW Hya and EG And have never had a recorded outburst while CQ Dra and AE Ara have outburst hi...
Far Ultraviolet Spectroscopy of Old Novae. II. RR Pic, V533 Her, and DI Lac [0.03%]
旧新星的远紫外光谱研究．第II部分：RR Pic、V533 Her和DI Lac
Edward M Sion,Patrick Godon,Liam Jones
Edward M Sion
The old novae V533 Her (Nova Her 1963), DI Lac (Nova Lac 1910), and RR Pic (Nova Pic 1891) are in (or near) their quiescent stage, following their nova explosions, and continue to accrete at a high rate in the aftermath of their explosions....
Edward M Sion,Patrick Godon,Alexandra Bisol
Edward M Sion
We present the results of a synthetic spectral analysis of the far ultraviolet archival IUE, HST and FUSE observations of the fast old nova V603 Aql, obtained some 90 years after its 1918 nova outburst. Our analysis utilizes the new Hubble ...
Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence? [0.03%]
CW Mon的矮新星的哈勃COS分光观测：静寂状态下的白矮星？
Connor Hause,Edward M Sion,Patrick Godon et al.
Connor Hause et al.
We present a synthetic spectral analysis of the HST COS spectrum of the U Geminorum-type dwarf nova CW Mon, taken during quiescence as part of our COS survey of accreting white dwarfs in Cataclysmic Variables. We use synthetic photosphere a...