Search Publications

First detections of H13CO+ and HC15N in the disk around HD 97048. Evidence for a cold gas reservoir in the outer disk
DOI: 10.1051/0004-6361/201834388 Bibcode: 2019A&A...629A..75B

Booth, Alice S.; Ilee, John D.; Walsh, Catherine

Observations of different molecular lines in protoplanetary disks provide valuable information on the gas kinematics, as well as constraints on the radial density and temperature structure of the gas. With ALMA we have detected H13CO+ (J = 4-3) and HC15N (J = 4-3) in the HD 97048 protoplanetary disk for the first t…

2019 Astronomy and Astrophysics
Gaia 16
The HADES RV programme with HARPS-N at TNG. XI. GJ 685 b: a warm super-Earth around an active M dwarf
DOI: 10.1051/0004-6361/201834969 Bibcode: 2019A&A...625A.126P

Rebolo, R.; Ribas, I.; Scandariato, G. +23 more

Context. Small rocky planets seem to be very abundant around low-mass M-type stars. Their actual planetary population is however not yet precisely understood. Currently, several surveys aim to expand the statistics with intensive detection campaigns, both photometric and spectroscopic.
Aims: The HADES program aims to improve the current stati…

2019 Astronomy and Astrophysics
Gaia 16
Discovery of kilogauss magnetic fields on the nearby white dwarfs WD 1105-340 and WD 2150+591
DOI: 10.1051/0004-6361/201834638 Bibcode: 2019A&A...623A..46L

Bagnulo, S.; Landstreet, J. D.

Magnetic fields are present in roughly 10% of white dwarfs. These fields affect the structure and evolution of such stars, and may provide clues about their earlier evolution history. Particularly important for statistical studies is the collection of high-precision spectropolarimetric observations of (1) complete magnitude-limited samples and (2)…

2019 Astronomy and Astrophysics
Gaia 16
Carbon and Oxygen Isotopic Ratios. II. Semiregular Variable M Giants
DOI: 10.3847/1538-4357/ab4e9b Bibcode: 2019ApJ...886..117L

Pilachowski, Catherine A.; Lambert, David L.; Hinkle, Kenneth H. +3 more

Carbon and oxygen isotopic ratios are reported for a sample of 51 SRb- and Lb-type variable asymptotic giant branch stars. Vibration-rotation first- and second-overtone CO lines in 1.5-2.5 µm spectra were measured to derive isotopic ratios for 12C/13C, 16O/17O, and 16O/18O. Co…

2019 The Astrophysical Journal
Gaia 16
The Substructures in the Local Stellar Halo from Gaia and LAMOST
DOI: 10.3847/1538-4357/ab06f4 Bibcode: 2019ApJ...874...74L

Donlon, Thomas; Du, Cuihua; Li, Hefan +2 more

Based on the second Gaia data release and spectroscopy from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope Data, we identified 20,089 halo stars kinematically and chemically. The halo streams in the solar neighborhood could be detected in the space of energy and angular momentum. We reshuffle the velocities of these stars to determi…

2019 The Astrophysical Journal
Gaia 16
Combined geometrical modelling and white-light mass determination of coronal mass ejections
DOI: 10.1051/0004-6361/201833829 Bibcode: 2019A&A...623A.139P

Vourlidas, Angelos; Bothmer, Volker; Pluta, Adam +2 more

Context. We use forward modelling on multi-viewpoint coronagraph observations to estimate the 3-dimensional morphology, initial speed and deprojected masses of Coronal Mass Ejections (CMEs). The CME structure is described via the Graduated Cylindrical Shell (GCS) model, which enables the measurement of CME parameters in a consistent and comparable…

2019 Astronomy and Astrophysics
SOHO 16
High- and Low-α Disk Stars Separate Dynamically at All Ages
DOI: 10.3847/1538-4357/ab2981 Bibcode: 2019ApJ...880..134G

Ness, Melissa K.; Gandhi, Suroor S.

There is a dichotomy in the Milky Way in the [α/Fe]-[Fe/H] plane, in which stars fall into high-α and low-α sequences. The high-α sequence comprises mostly old stars, and the low-α sequence comprises primarily young stars. The origin of this dichotomy is uncertain. To better understand how the high- and low-α stars are affiliated, we examine if th…

2019 The Astrophysical Journal
Gaia 16
Probing Structure in Cold Gas at z ≲ 1 with Gravitationally Lensed Quasar Sight Lines
DOI: 10.3847/1538-4357/ab4c2e Bibcode: 2019ApJ...886...83K

Ellison, Sara L.; Kulkarni, Varsha P.; Lopez, Sebastian +3 more

Absorption spectroscopy of gravitationally lensed quasars (GLQs) enables study of spatial variations in the interstellar and/or circumgalactic medium of foreground galaxies. We report observations of four GLQs, each with two images separated by 0.″8-3.″0, that show strong absorbers at redshifts 0.4 < z abs < 1.3 in their spectra, …

2019 The Astrophysical Journal
eHST 16
The visual spectrum of Jupiter's Great Red Spot accurately modeled with aerosols produced by photolyzed ammonia reacting with acetylene
DOI: 10.1016/j.icarus.2019.04.008 Bibcode: 2019Icar..330..217B

Baines, K. H.; Sromovsky, L. A.; Carlson, R. W. +2 more

We report results incorporating the optical properties of the red-tinted photochemically-generated aerosols of Carlson et al. (2016, Icarus 274, 106-115) in spectral models of Jupiter's Great Red Spot (GRS). This material - created in laboratory GRS simulations from acetylene reacting with photolytic products of ammonia produced by 0.2-µm ra…

2019 Icarus
eHST 16
From ridges in the velocity distribution to wiggles in the rotation curve
DOI: 10.1093/mnrasl/slz042 Bibcode: 2019MNRAS.485L.104M

Martinez-Medina, Luis; Pichardo, Barbara; Peimbert, Antonio +1 more

Recently, the Gaiadata release 2 (DR2) showed us the richness in the kinematics of the Milky Way disc. Of particular interest is the presence of ridges covering the stellar velocity distribution, Vϕ-R; as shown by others, it is likely that these ridges are the signature of phase mixing, transient spirals, or the bar. Here, with a Galact…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 16