Search Results - "Liu, X W"
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The Milky Way's rotation curve out to 100 kpc and its constraint on the Galactic mass distribution
Published in Monthly notices of the Royal Astronomical Society (11-12-2016)“…The rotation curve (RC) of the Milky Way out to ~100 kpc has been constructed using ~16,000 primary red clump giants (PRCGs) in the outer disc selected from…”
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Empirical extinction coefficients for the GALEX, SDSS, 2MASS and WISE passbands
Published in Monthly notices of the Royal Astronomical Society (11-04-2013)“…By using the 'standard pair' technique of pairing stars of almost nil and high extinction but otherwise with almost identical stellar parameters from the Sloan…”
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3
Empirical metallicity-dependent calibrations of effective temperature against colours for dwarfs and giants based on interferometric data
Published in Monthly notices of the Royal Astronomical Society (11-12-2015)“…We present empirical metallicity-dependent calibrations of effective temperature against colours for dwarfs of luminosity classes IV and V and for giants of…”
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Determination of the local standard of rest using the LSS-GAC DR1
Published in Monthly notices of the Royal Astronomical Society (01-05-2015)“…We re-estimate the peculiar velocity of the Sun with respect to the local standard of rest (LSR) using a sample of local stars within 600 pc of the Sun,…”
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Very deep spectroscopy of the bright Saturn nebula NGC7009 - I. Observations and plasma diagnostics
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…ABSTRACT We present very deep CCD spectrum of the bright, medium-excitation planetary nebula NGC7009, with a wavelength coverage from 3040 to 11000Å…”
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White dwarf–main sequence binaries from LAMOST: the DR5 catalogue
Published in Monthly notices of the Royal Astronomical Society (01-07-2018)“…Abstract We present the data release (DR) 5 catalogue of white dwarf–main sequence (WDMS) binaries from the Large sky Area Multi-Object fibre Spectroscopic…”
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Three-dimensional Distribution of the Interstellar Dust in the Milky Way
Published in The Astrophysical journal (01-01-2021)“…We present a three-dimensional (3D) extinction map of the southern sky. The map covers the SkyMapper Southern Survey (SMSS) area of ∼14,000 deg2 and has…”
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The Galactic spiral structure as revealed by O- and early B-type stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)Get full text
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9
Emulating Anyonic Fractional Statistical Behavior in a Superconducting Quantum Circuit
Published in Physical review letters (09-09-2016)“…Anyons are exotic quasiparticles obeying fractional statistics, whose behavior can be emulated in artificially designed spin systems. Here we present an…”
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Estimating stellar atmospheric parameters, absolute magnitudes and elemental abundances from the LAMOST spectra with Kernel-based principal component analysis
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…Accurate determination of stellar atmospheric parameters and elemental abundances is crucial for Galactic archaeology via large-scale spectroscopic surveys. In…”
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11
Elemental abundances of Galactic bulge planetary nebulae from optical recombination lines
Published in Monthly notices of the Royal Astronomical Society (21-10-2007)“…Deep long-slit optical spectrophotometric observations are presented for 25 Galactic bulge planetary nebulae (GBPNe) and six Galactic disc planetary nebulae…”
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12
Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. V. On the Origin of the "Young" [ /Fe]-enhanced Stars
Published in The Astrophysical journal (01-11-2020)“…Using a sample of nearly 140,000 primary red-clump stars selected from the LAMOST and Gaia surveys, we have identified a large sample of "young" […”
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13
Very deep spectroscopy of the bright Saturn nebula NGC 7009 - II. Analysis of the rich optical recombination spectrum
Published in Monthly notices of the Royal Astronomical Society (11-03-2013)“…In Paper I, we presented a deep, long-slit spectrum of the bright Saturn nebula NGC 7009. Numerous permitted lines emitted by the C+, N+, O+ and Ne+ ions were…”
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LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC): target selection and the first release of value-added catalogues
Published in Monthly notices of the Royal Astronomical Society (21-03-2015)“…As a major component of the LAMOST Galactic surveys, the LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC) aims to survey a significant volume…”
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Very Large Telescope deep echelle spectroscopy of Galactic planetary nebulae NGC 6153, M 1-42 and Hf 2-2
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…We present deep spectroscopy of three Galactic planetary nebulae (PNe) with large abundance discrepancy factors: NGC 6153, M 1-42 and Hf 2-2. The spectra were…”
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LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC): the second release of value-added catalogues
Published in Monthly notices of the Royal Astronomical Society (01-05-2017)“…Abstract We present the second release of value-added catalogues of the LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC DR2). The catalogues…”
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Mapping the three-dimensional dust extinction towards the supernova remnant S147 – the S147 dust cloud
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract We present a three-dimensional (3D) extinction analysis in the region towards the supernova remnant (SNR) S147 (G180.0–1.7) using multiband…”
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On the Kinematic Signature of the Galactic Warp As Revealed By the LAMOST-TGAS Data
Published in The Astrophysical journal (10-09-2018)“…Using a sample of about 123,000 stars with accurate 3D velocity measurements from the LAMOST-TGAS data, we confirm the kinematic signature of the Galactic warp…”
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Dusty Disks Around White Dwarfs. I. Origin of Debris Disks
Published in The Astrophysical journal (01-06-2010)“…A significant fraction of the mature FGK stars have cool dusty disks at least an order of magnitude brighter than the solar system's outer zodiacal light…”
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The age–metallicity relation in the solar neighbourhood from a pilot sample of white dwarf–main sequence binaries
Published in Monthly notices of the Royal Astronomical Society (01-12-2016)“…The age-metallicity relation (AMR) is a fundamental observational constraint for understanding how the Galactic disc formed and evolved chemically in time…”
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