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Related papers: Polarization Studies of Comet C/2000 WM1 (LINEAR)

200 papers

Ultra-cool dwarfs of the L spectral type (Teff=1400-2200K) are known to have dusty atmospheres. Asymmetries of the dwarf surface may arise from rotationally-induced flattening and dust-cloud coverage, and may result in non-zero linear…

Solar and Stellar Astrophysics · Physics 2015-05-13 B. Goldman , J. Pitann , M. R. Zapatero Osorio , C. A. L. Bailer-Jones , V. J. S. Bejar , J. A. Caballero , Th. Henning

We detected with the IRAM interferometer the lines of CO(4-3) and CO(9-8) from the recently-discovered broad absorption line quasar APM 08279+5255. The molecular lines are at a redshift of 3.911, which we take to be the true cosmological…

Astrophysics · Physics 2009-10-31 D. Downes , R. Neri , T. Wiklind , D. J. Wilner , P. Shaver

We report results based on mid-infrared photometry of comet 103P/Hartley 2 taken during May 4-13, 2010 (when the comet was at a heliocentric distance of 2.3 AU, and an observer distance of 2.0 AU) by the Wide-field Infrared Survey Explorer…

We present 870 $\mu$m ALMA dust polarization observations of 10 young Class 0/I protostars in the Perseus Molecular Cloud. At $\sim$ 0.35$"$ (80 au) resolution, all of our sources show some degree of polarization, with most (9/10) showing…

Solar and Stellar Astrophysics · Physics 2018-03-28 Erin G. Cox , Robert J. Harris , Leslie W. Looney , Zhi-Yun Li , Haifeng Yang , John J. Tobin , Ian Stephens

We present our results for comet (ISON). Our results were obtained with amateur telescopes observing from the ground, before and after the comet had passed conjunction with the Sun in August 2013. We measured a mean radius of 830 +- 245 m,…

Solar and Stellar Astrophysics · Physics 2014-05-14 Toni Scarmato

Science opportunities and recommendations concerning optical/infrared polarimetry for the upcoming decade in the field of cosmology. Community-based White Paper to Astro2010 in response to the call for such papers.

We report the discovery of X-ray emission from comet C/1995 O1 (Hale-Bopp) by the LECS instrument on-board BeppoSAX on 1996 September 10--11. The 0.1--2.0 keV luminosity decayed by a factor of 2 on a timescale of ~10 hr with a mean value of…

We imaged Comet 252P/2000 G1 (LINEAR) (hereafter 252P) with the Hubble Space Telescope and both 252P and P/2016 BA$_{14}$ (PanSTARRS) (hereafter BA$_{14}$) with the Discovery Channel Telescope in March and April 2016, surrounding its close…

During its sungrazing perihelion passage, comet ISON appeared in the field of view of the SUMER spectrometer and allowed unique observations at far-ultraviolet wavelengths with high spatial and temporal resolution. We report results of…

Solar and Stellar Astrophysics · Physics 2015-06-22 W. Curdt , H. Boehnhardt , J. -B. Vincent , S. K. Solanki , U. Schühle , L. Teriaca

The galaxy M51 was observed using the Mimir instrument on the Perkins telescope to constrain the resolved H-band (1.6 $\mu$m) polarization across the galaxy. These observations place an upper limit of $P_H<0.05%$ on the $H$-band…

Astrophysics of Galaxies · Physics 2015-06-12 Michael D. Pavel , Dan P. Clemens

We present an analysis of long-slit cometary spectroscopy using the dual-arm ISIS spectrograph on the 4.2 m WHT. Eleven comets were observed over two nights in 2016 March and we detected the OH (0-0) emission band at 3085 {\AA} in the…

Earth and Planetary Astrophysics · Physics 2019-01-16 Méabh Hyland , Alan Fitzsimmons , Colin Snodgrass

The eccentric WR+O binary system WR 140 produces dust for a few months at intervals of 7.94 yrs coincident with periastron passage. We present the first resolved images of this dust shell, at binary phases ~0.039 and ~0.055, using aperture…

Astrophysics · Physics 2009-11-07 J. D. Monnier , P. G. Tuthill , W. C. Danchi

Observations of the sungrazing comet C/2012 S1 (ISON) were carried out using the Atacama Large Millimeter/submillimeter Array (ALMA) at a heliocentric distance of 0.58-0.54 AU (pre-perihelion) on 2013 November 16-17. Temporally resolved…

We present new spectra of WR 140 (HD 193793) in the JHK bands with some covering the 1.083-micron He I emission line at higher resolution, observed between 2000 October and 2003 May to cover its 2001 periastron passage. The WC7 + O4-5…

Astrophysics · Physics 2009-11-10 W. P. Varricatt , P. M. Williams , N. M. Ashok

We present an analysis of polarised dust emission at 850 micron for a parsec long filament in the northern part of the Orion B molecular cloud. The region was observed by the JCMT SCUBA-2/POL-2 polarimeter. The filament has a line mass (~80…

We report on high spectral resolution observations of comet C/1999 S4 (LINEAR) obtained at McDonald Observatory in June and July 2000. We report unequivocal detections of the O (1S) and O (1D) metastable lines in emission in the cometary…

Astrophysics · Physics 2009-11-07 Anita L. Cochran , William D. Cochran

The measurement of polarization of the background stars in the region of Bok globules is important to study the magnetic field geometry and dust grain characteristics in the globule. These parameters are important for the formation and…

Instrumentation and Methods for Astrophysics · Physics 2012-06-08 D. Paul , H. S. Das , A. K. Sen

We report on polarimetric observations of 100 pulsars centered on 774 MHz, made using the Green Bank Telescope, presenting their polarization profiles and polarized flux densities and comparing them with previous observations when possible.…

Solar and Stellar Astrophysics · Physics 2009-03-25 J. L. Han , P. B. Demorest , W. van Straten , A. G. Lyne

We present optical observations of two remarkable new AGN discovered by the Two-Micron All Sky Survey. Both are classified as QSOs based on their optical spectra, near-IR colors, and near-IR and [O III]5007 luminosities, but their optical…

Astrophysics · Physics 2007-05-23 P. S. Smith , G. D. Schmidt , D. C. Hines , R. M. Cutri , B. O. Nelson

We report on photometry and high resolution spectroscopy of the chemically peculiar Jupiter-family Comet (hereafter JFC) 21P/Giacobini-Zinner. Comet 21P is a well known member of the carbon-chain depleted family but displays also a…

Earth and Planetary Astrophysics · Physics 2020-08-12 Y. Moulane , E. Jehin , P. Rousselot , J. Manfroid , Y. Shinnaka , F. J. Pozuelos , D. Hutsemékers , C. Opitom , B. Yang , Z. Benkhaldoun