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HD 96446: a long-period binary with a strongly magnetic He-rich primary with β Cephei pulsations
DOI: 10.1051/0004-6361/201935177 Bibcode: 2019A&A...626A..94G

Järvinen, S.; González, J. F.; Butler, K. +14 more


Aims: HD 96446 is a magnetic B2p He-strong star that has been reported to be a β Cep pulsator. We present a detailed spectroscopic analysis of this object based on an intensive observational data set obtained in a multisite campaign with the spectrographs CORALIE, FEROS, and HARPS (La Silla); UVES (Paranal); HERCULES (Mt. John Observatory); a…

2019 Astronomy and Astrophysics
Gaia IUE 11
Extended star-forming regions within galaxies in a dense proto-cluster core at z = 2.53
DOI: 10.1093/pasj/psz047 Bibcode: 2019PASJ...71...69S

Suzuki, Tomoko L.; Minowa, Yosuke; Koyama, Yusei +5 more

At z ∼ 2, star formation activity is thought to be high even in high-density environments such as galaxy clusters and proto-clusters. One of the critical but outstanding issues is if the structural growth of star-forming galaxies can differ depending on their surrounding environments. In order to investigate how galaxies grow their structures and …

2019 Publications of the Astronomical Society of Japan
eHST 11
Evidence of Hubble Flow-like Motion of Young Stellar Populations away from the Perseus Arm
DOI: 10.3847/2041-8213/aafb06 Bibcode: 2019ApJ...871L..12R

Hernández, Jesús; Roman-Lopes, Alexandre; Tapia, Mauricio +2 more

In this Letter we present evidence of the coherent outward motion of a sample of young stars (t < 30 Myr) in the Perseus Arm, whose apparent origin is located in the vicinity of the W3/W4/W5 complex. Using astrometric and photometric data from the Gaia Data Release 2 catalog of an 8 radius field centered near W4, we selected a sampl…

2019 The Astrophysical Journal
Gaia 11
A Search for Variable Stars in the Globular Cluster M4 with K2
DOI: 10.3847/1538-4365/ab3849 Bibcode: 2019ApJS..244...12W

Wallace, Joshua J.; Hartman, Joel D.; Bakos, Gáspár Á. +1 more

We extract light curves for 4554 objects with 9 < G < 19 in the K2 superstamp observations of the globular cluster M4, including 3784 cluster members, and search for variability. Among cluster-member objects, we detect 66 variables, of which 52 are new discoveries. Among objects not belonging to the cluster, we detect 24 variables, of which …

2019 The Astrophysical Journal Supplement Series
Gaia 11
The 3D shape of Type IIb SN 2011hs
DOI: 10.1093/mnras/stz265 Bibcode: 2019MNRAS.485..102S

Spyromilio, J.; Wang, L.; Wheeler, J. C. +10 more

We observed seven epochs of spectropolarimetry in optical wavelengths for the Type IIb SN 2011hs, ranging from -3 to +40 d with respect to V-band maximum. A high degree of interstellar polarization was detected (up to ∼3 per cent), with a peak lying blueward of 4500 Å. Similar behaviours have been seen in some Type Ia supernovae (SNe), but had nev…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 11
Observations of Asymmetric Lobe Convection for Weak and Strong Tail Activity
DOI: 10.1029/2019JA026773 Bibcode: 2019JGRA..124.9999O

Østgaard, N.; Tenfjord, P.; Reistad, J. P. +6 more

In this study we use high-quality convection data from the Electron Drift Instrument on board Cluster to investigate how near-Earth tail activity affects the average convection pattern in the magnetotail lobes when the interplanetary magnetic field has a dominating east-west (By) component. Two different proxies have been used to repres…

2019 Journal of Geophysical Research (Space Physics)
Cluster 11
Discovery of a giant and luminous Lyα+C IV+He II nebula at z = 3.326 with extreme emission line ratios
DOI: 10.1051/0004-6361/201936013 Bibcode: 2019A&A...629A..23M

Pérez-Fournon, I.; Ivison, R. J.; Omont, A. +17 more

We present the discovery of HLock01-LAB, a luminous and large Lyα nebula at z = 3.326. Medium-band imaging and long-slit spectroscopic observations with the Gran Telescopio Canarias reveal extended emission in the Lyα 1215 Å, C IV 1550 Å, and He II 1640 Å lines over ∼100 kpc, and a total luminosity LLyα = (6.4 ± 0.1)×1044 erg…

2019 Astronomy and Astrophysics
Gaia eHST 11
The extreme O-type spectroscopic binary HD 93129A. A quantitative, multiwavelength analysis
DOI: 10.1051/0004-6361/201833178 Bibcode: 2019A&A...621A..63G

Gruner, D.; Hamann, W. -R.; Oskinova, L. M. +6 more

Context. HD 93129A was classified as the earliest O-type star in the Galaxy (O2 If*) and is considered as the prototype of its spectral class. However, interferometry shows that this object is a binary system, while recent observations even suggest a triple configuration. None of the previous spectral analyses of this object accounted for its mult…

2019 Astronomy and Astrophysics
Gaia eHST 11
Multiple Stellar Populations of Globular Clusters from Homogeneous Ca-CN-CH Photometry. V. {{cn}}_{JWL}}^{{\prime} } as a Surrogate cn JWL Index and NGC 6723
DOI: 10.3847/1538-4357/ab3d34 Bibcode: 2019ApJ...883..166L

Lee, Jae-Woo

We introduce new color indices {{cn}}JWL}{\prime } (=Ca CTIO - Ca JWL) and ch JWL [=(JWL43 - b) - (b - y)], accurate photometric measures of the CN band at λ3883 and the CH G band, respectively, in the study of the multiple populations (MPs) in globular clusters (GCs). Our photometric CN-CH re…

2019 The Astrophysical Journal
Gaia 11
Validation of the IPSL Venus GCM Thermal Structure with Venus Express Data
DOI: 10.3390/atmos10100584 Bibcode: 2019Atmos..10..584S

Piccioni, Giuseppe; Tellmann, Silvia; Lebonnois, Sebastien +4 more

General circulation models (GCMs) are valuable instruments to understand the most peculiar features in the atmospheres of planets and the mechanisms behind their dynamics. Venus makes no exception and it has been extensively studied thanks to GCMs. Here we validate the current version of the Institut Pierre Simon Laplace (IPSL) Venus GCM, by means…

2019 Atmosphere
VenusExpress 11