Search Publications

Pulsational properties of ten new slowly pulsating B stars
DOI: 10.1051/0004-6361/201935478 Bibcode: 2020A&A...633A.122F

Paunzen, E.; Fedurco, M.; Bernhard, K. +2 more

Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show non-radial g-mode oscillations driven by the κ mechanism acting on the iron bump. These multi-periodic pulsators have great asteroseismic potential and can be employed for the calibration of stellar structure and evolution models of massive stars.

2020 Astronomy and Astrophysics
Gaia INTEGRAL 9
Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph
DOI: 10.1093/mnras/staa1422 Bibcode: 2020MNRAS.495.3482A

Bond, J. Richard; Hensley, Brandon S.; Casassus, Simon +9 more

The ρ Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ρ Oph W, the PDR exposed to B-type star HD 147889, and highlight the absence of signal from S1, the brightest IR nebula in the c…

2020 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 9
Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects. II
DOI: 10.3847/1538-3881/ab6ded Bibcode: 2020AJ....159..114O

Oliveira, A. S.; Rodrigues, C. V.; Martins, M. +4 more

This is the second paper of a series presenting our search for magnetic cataclysmic variables (mCVs) among candidates selected mostly from the Catalina Real-Time Transient Survey. We present the identification spectra, obtained at the SOAR Telescope, as well as magnitudes and Gaia distances for 45 objects. Of these, 39 objects are identified as CV…

2020 The Astronomical Journal
Gaia XMM-Newton 9
Extreme ultraviolet quasar colours from GALEX observations of the SDSS DR14Q catalogue
DOI: 10.1093/mnras/staa411 Bibcode: 2020MNRAS.493.2745V

Wu, Jian; Vanden Berk, Daniel E.; Wesolowski, Sarah C. +4 more

The rest-frame far to extreme ultraviolet (UV) colour-redshift relationship has been constructed from data on over $480\, 000$ quasars carefully cross-matched between SDSS Data Release 14 and the final GALEX photometric catalogue. UV matching and detection probabilities are given for all the quasars, including dependencies on separation, optical b…

2020 Monthly Notices of the Royal Astronomical Society
eHST 9
Feedback of molecular outflows from protostars in NGC 1333 revealed by Herschel and Spitzer spectro-imaging observations
DOI: 10.1051/0004-6361/202037684 Bibcode: 2020A&A...641A..36D

Güdel, Manuel; Persson, Magnus; Tafalla, Mario +2 more

Context. Far infrared cooling of excited gas around protostars has been predominantly studied in the context of pointed observations. Large-scale spectral maps of star forming regions enable the simultaneous, comparative study of the gas excitation around an ensemble of sources at a common frame of reference, therefore, providing direct insights i…

2020 Astronomy and Astrophysics
Herschel 9
Gas and star formation from HD and dust emission in a strongly lensed galaxy
DOI: 10.1093/mnras/staa2689 Bibcode: 2020MNRAS.498.4109J

Maiolino, R.; Caselli, P.; Carniani, S. +1 more

The molecular gas content of high-redshift galaxies is a highly sought-after property. However, H2 is not directly observable in most environments, so its mass is probed through other emission lines (e.g. CO, [C I], [C II]), or through a gas-to-dust ratio. Each of these methods depends on several assumptions, and are best used in parall…

2020 Monthly Notices of the Royal Astronomical Society
eHST 9
Clustering of Fast Coronal Mass Ejections during Solar Cycles 23 and 24 and the Implications for CME-CME Interactions
DOI: 10.3847/1538-4357/ab9e72 Bibcode: 2020ApJ...899...47R

Veronig, Astrid; Podladchikova, Tatiana; Feynman, Joan +3 more

We study the clustering properties of fast coronal mass ejections (CMEs) that occurred during solar cycles 23 and 24. We apply two methods: the Max Spectrum method can detect the predominant clusters, and the declustering threshold time method provides details on the typical clustering properties and timescales. Our analysis shows that during the …

2020 The Astrophysical Journal
SOHO 9
Component properties and mutual orbit of binary main-belt comet 288P/(300163) 2006 VW139
DOI: 10.1051/0004-6361/202038195 Bibcode: 2020A&A...643A.152A

Agarwal, J.; Weaver, H.; Larson, S. +3 more

Context. The binary asteroid 288P/(300163) is unusual both for its combination of wide-separation and high mass ratio and for its comet-like activity. It is not currently known whether there is a causal connection between the activity and the unusual orbit or if instead the activity helped to overcome a strong detection bias against such sub-arcse…

2020 Astronomy and Astrophysics
eHST 9
Illuminating a tadpole's metamorphosis II: observing the ongoing transformation with ALMA
DOI: 10.1093/mnras/staa1504 Bibcode: 2020MNRAS.496..394R

Reiter, Megan; Garay, Guido; McLeod, Anna F. +4 more

We present new Atacama Large Millimeter/submillimeter Array observations of the tadpole, a small globule in the Carina Nebula that hosts the HH 900 jet+outflow system. Our data include 12CO, 13CO, C18O J=2-1, 13CO, C18O J=3-2, and serendipitous detections of DCN J=3-2 and CS J=7-6. With angula…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 9
Two successive partial mini-filament confined ejections
DOI: 10.1016/j.asr.2019.09.026 Bibcode: 2020AdSpR..65.1629P

Mandrini, C. H.; Cristiani, G. D.; López Fuentes, M. +2 more

Active region (AR) NOAA 11476 produced a series of confined plasma ejections, mostly accompanied by flares of X-ray class M, from 08 to 10 May 2012. The structure and evolution of the confined ejections resemble that of EUV surges; however, their origin is associated to the destabilization and eruption of a mini-filament, which lay along the photo…

2020 Advances in Space Research
Hinode 9