Search Publications

Fast spectrophotometry of WD 1145+017
DOI: 10.1093/mnras/sty2315 Bibcode: 2018MNRAS.481..703I

Villaver, Eva; Raddi, Roberto; Gänsicke, Boris T. +16 more

WD 1145+017 is currently the only white dwarf known to exhibit periodic transits of planetary debris as well as absorption lines from circumstellar gas. We present the first simultaneous fast optical spectrophotometry and broad-band photometry of the system, obtained with the Gran Telescopio Canarias (GTC) and the Liverpool Telescope, respectively…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 32
SHARDS: constraints on the dust attenuation law of star-forming galaxies at z ∼ 2
DOI: 10.1093/mnras/stx3334 Bibcode: 2018MNRAS.475.2363T

Barro, Guillermo; Pérez-González, Pablo G.; Cava, Antonio +11 more

We make use of the Survey of High-z Absorption Red and Dead Sources, an ultradeep (<26.5AB) galaxy survey that provides optical photospectra at resolution R ∼ 50, via medium-band filters (FWHM ∼ 150 Å). This data set is combined with ancillary optical and NIR fluxes to constrain the dust attenuation law in the rest-frame NUV region of star-form…

2018 Monthly Notices of the Royal Astronomical Society
eHST 32
Constraining physical conditions for the PDR of Trumpler 14 in the Carina Nebula
DOI: 10.1051/0004-6361/201832595 Bibcode: 2018A&A...618A..53W

Onaka, Takashi; Okada, Yoko; Le Petit, Franck +5 more

We investigate the physical conditions of the CO gas, based on the submillimeter imaging spectroscopy from a 2' × 7' (1.5 × 5 pc2) area near the young star cluster, Trumpler 14 of the Carina Nebula. The observations presented in this work are taken with the Fourier Transform Spectrometer (FTS) of the Spectral and Photometric Imaging REc…

2018 Astronomy and Astrophysics
Herschel ISO 32
ALMA observation of the disruption of molecular gas in M87
DOI: 10.1093/mnras/sty047 Bibcode: 2018MNRAS.475.3004S

Simionescu, A.; Allen, S. W.; Werner, N. +3 more

We present the results from Atacama Large Millimeter Array (ALMA) observations centred 40 arcsec (3 kpc in projection) south-east of the nucleus of M87. We report the detection of extended CO (2-1) line emission with a total flux of (5.5 ± 0.6) × 10-18 erg s-1 cm-2 and corresponding molecular gas mass M_{H_2}=(4.7 …

2018 Monthly Notices of the Royal Astronomical Society
eHST 31
Planck Cold Clumps in the λ Orionis Complex. II. Environmental Effects on Core Formation
DOI: 10.3847/1538-4365/aac2e0 Bibcode: 2018ApJS..236...51Y

Ristorcelli, I.; Soam, Archana; Choi, Minho +29 more

Based on the 850 µm dust continuum data from SCUBA-2 at James Clerk Maxwell Telescope (JCMT), we compare overall properties of Planck Galactic Cold Clumps (PGCCs) in the λ Orionis cloud to those of PGCCs in the Orion A and B clouds. The Orion A and B clouds are well-known active star-forming regions, while the λ Orionis cloud has a different…

2018 The Astrophysical Journal Supplement Series
AKARI Planck 31
The radius of the quiescent neutron star in the globular cluster M13
DOI: 10.1093/mnras/sty582 Bibcode: 2018MNRAS.476.4713S

Campana, S.; Heinke, C. O.; Cohn, H. N. +5 more

X-ray spectra of quiescent low-mass X-ray binaries containing neutron stars can be fit with atmosphere models to constrain the mass and the radius. Mass-radius constraints can be used to place limits on the equation of state of dense matter. We perform fits to the X-ray spectrum of a quiescent neutron star in the globular cluster M13, utilizing da…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
Exploring the space density of X-ray selected cataclysmic variables
DOI: 10.1051/0004-6361/201833723 Bibcode: 2018A&A...619A..62S

Schwope, A. D.

The space density of the various classes of cataclysmic variables (CVs) has up to now only been weakly constrained, due to the small number of objects in complete X-ray flux-limited samples and the difficulty in deriving precise distances to CVs. The former limitation still exists. Here the impact of Gaia parallaxes and implied distances on the sp…

2018 Astronomy and Astrophysics
Gaia 31
On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic H I
DOI: 10.3847/1538-4357/aad8ac Bibcode: 2018ApJ...864..132B

Tripp, Todd M.; Prochaska, J. Xavier; Tumlinson, Jason +3 more

We analyze the equivalent widths of H I {{Ly}}α ({W}Lyα }) absorption from the inner (R < 160 kpc) circumgalactic medium (CGM) of 85 galaxies at z ∼ 0 with stellar masses M * ranging 8≤slant {log} {M}* /{M}≤slant 11.6. Across three orders of magnitude in stellar mass, the CGM of present-day galaxies…

2018 The Astrophysical Journal
eHST 31
Large-Scale Survey of the Structure of the Dayside Magnetopause by MMS
DOI: 10.1002/2017JA025121 Bibcode: 2018JGRA..123.2018P

Russell, C. T.; Lavraud, B.; Baumjohann, W. +13 more

This paper describes the generation and initial utilization of a database containing 80 vector and scalar quantities, for a total of 8,670 magnetopause and magnetosheath current sheet crossings by MMS1, using plasma and magnetic field data from the Fast Plasma Investigation, Fluxgate Magnetometer, and Hot Plasma Composition Analyzer instruments, a…

2018 Journal of Geophysical Research (Space Physics)
Cluster 31
A Tale of “Two” Comets: The Primary Volatile Composition of Comet 2P/Encke Across Apparitions and Implications for Cometary Science
DOI: 10.3847/1538-3881/aae0f7 Bibcode: 2018AJ....156..251R

Vervack, Ronald J., Jr.; Kawakita, Hideyo; DiSanti, Michael A. +5 more

The highly favorable 2017 apparition of 2P/Encke allowed the first comprehensive comparison of primary volatile abundances in a given comet across multiple apparitions. This apparition offered opportunities to address pressing questions in cometary science, including investigating evolutionary and/or heliocentric distance (R h) effects …

2018 The Astronomical Journal
Rosetta 31