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...
A SEARCH FOR LOST PLANETS IN THE KEPLER MULTI-PLANET SYSTEMS AND THE DISCOVERY OF A LONG PERIOD, NEPTUNE-SIZED EXOPLANET KEPLER-150 F [0.03%]
开普勒多行星系统中的寻找丢失的系外行星以及关于类海王星系外行星开普勒150f的发现
Joseph R Schmitt,Jon M Jenkins,Debra A Fischer
Joseph R Schmitt
The vast majority of the 4700 confirmed planets and planet candidates discovered by the Kepler space telescope were first found by the Kepler pipeline. In the pipeline, after a transit signal is found, all data points associated with those ...
A W Meyer,R G Smith,S B Charnley et al.
A W Meyer et al.
In an attempt to better understand the conditions under which molecules condense onto grains in the envelopes of evolved stars, we have searched for the presence of H2O ice in the circumstellar envelopes of several evolved (OH/IR) stars. Th...
S C Madden,W M Irvine,H E Matthews et al.
S C Madden et al.
We report the results of an initial survey in a variety of Galactic sources for cyclopropenylidene (C3H2), the first interstellar hydrocarbon ring molecule. C3H2 is found to be very widespread throughout the Galaxy. This, together with its ...
Comet Sugano-Saigusa-Fujikawa (1983V)--a small, puzzling comet [0.03%]
小而令人迷惑的 Sugano-Saigusa-Fujikawa 彗星(1983 V)
M S Hanner,R L Newburn,H Spinrad et al.
M S Hanner et al.
Spectroscopic and infrared observations of Comet Sugano-Saigusa-Fujikawa (1983V) were obtained during its close approach to the Earth on 11-14 June 1983. The [O I] production rates of 1.8 +/- 0.9 x 10(26) atoms/s observed on 12.3 June and 7...
G J Veeder,M S Hanner,D L Matson et al.
G J Veeder et al.
We report 10 micrometers infrared photometry for 22 Aten, Apollo, and Amor asteroids. Thermal models are used to derive the corresponding radiometric albedos and diameters. Several of these asteroids appear to have surfaces of relatively hi...
M S Hanner,G J Veeder,A T Tokunaga
M S Hanner
We present 1-20 micrometers photometry of P/Giacobini-Zinner obtained at the NASA Infrared Telescope Facility, during 1985 June-September (r = 1.57-1.03 AU). A broad, weak 10 micrometers silicate emission feature was detected on August 26.6...