Search Publications

Formation of Radio Type II Bursts During a Multiple Coronal Mass Ejection Event
DOI: 10.1007/s11207-017-1208-y Bibcode: 2017SoPh..292..183A

Valtonen, Eino; Pohjolainen, Silja; Al-Hamadani, Firas

We study the solar event on 27 September 2001 that consisted of three consecutive coronal mass ejections (CMEs) originating from the same active region, which were associated with several periods of radio type II burst emission at decameter-hectometer (DH) wavelengths. Our analysis shows that the first radio burst originated from a low-density env…

2017 Solar Physics
SOHO 3
Photometric and spectroscopic variability of the B5IIIe star HD 171219
DOI: 10.1051/0004-6361/201629177 Bibcode: 2017A&A...603A..41A

Poretti, E.; Rainer, M.; Uytterhoeven, K. +11 more

We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type, whose spectra show, or have shown at some epoch, Balmer lines in emission and an infrared excess.…

2017 Astronomy and Astrophysics
CoRoT 3
Statistical survey of day-side magnetospheric current flow using Cluster observations: magnetopause
DOI: 10.5194/angeo-35-645-2017 Bibcode: 2017AnGeo..35..645L

Fornaçon, Karl-Heinz; Glassmeier, Karl-Heinz; Liebert, Evelyn +2 more

We present a statistical survey of current structures observed by the Cluster spacecraft at high-latitude day-side magnetopause encounters in the close vicinity of the polar cusps. Making use of the curlometer technique and the fluxgate magnetometer data, we calculate the 3-D current densities and investigate the magnetopause current direction, lo…

2017 Annales Geophysicae
Cluster 3
Dual E × B flow responses in the dayside ionosphere to a sudden IMF By rotation
DOI: 10.1002/2017GL073374 Bibcode: 2017GeoRL..44.6525E

Trattner, K. J.; Eriksson, S.; Baker, J. B. H. +3 more

We report for the first time a dual transition state in the dayside ionosphere following a sudden rotation of the interplanetary magnetic field (IMF) in the upstream magnetosheath from IMF <fi>B</fi><fi>y</fi> < 0 to <fi>B</fi><fi>y</fi> > 0 during <fi>B</fi>

2017 Geophysical Research Letters
Cluster 3
The dusty silhouette jet HH 1019 in the Carina Nebula
DOI: 10.1093/mnras/stx386 Bibcode: 2017MNRAS.467.4441R

Smith, Nathan; Bally, John; Reiter, Megan +1 more

We report the discovery in Hubble Space Telescope (HST) images of the new Herbig-Haro jet, HH 1019, located near the Tr 14 cluster in the Carina Nebula. Like other HH jets in the region, this bipolar collimated flow emerges from the head of a dark dust pillar. However, HH 1019 is unique because - unlike all other HH jets known to date - it is iden…

2017 Monthly Notices of the Royal Astronomical Society
eHST 3
A deep staring campaign in the σ Orionis cluster. Variability in substellar members
DOI: 10.1051/0004-6361/201730973 Bibcode: 2017A&A...608A..66E

Eislöffel, J.; Scholz, A.; Jayawardhana, R. +2 more

Context. The young star cluster near σ Orionis is one of the primary environments to study the properties of young brown dwarfs down to masses comparable to those of giant planets.
Aims: Deep optical imaging is used to study time-domain properties of young brown dwarfs over typical rotational timescales and to search for new substellar and pl…

2017 Astronomy and Astrophysics
Gaia 3
X-ray studies of solar system objects: Past, present, and the next decade
DOI: 10.1002/asna.201713329 Bibcode: 2017AN....338..188B

Branduardi-Raymont, G.

This paper presents an overview of the remarkable progress that X-ray studies of solar system objects have delivered over the past three decades, covering research that encompasses remote observations with XMM-Newton and Chandra, in situ measurements by planetary missions, and models of solar wind propagation from 1 AU. The future of X-ray explora…

2017 Astronomische Nachrichten
XMM-Newton 3
A broad spectral feature detected during the cooling phase of a type I X-ray burst from GRS 1747-312 with Suzaku
DOI: 10.1093/pasj/psx037 Bibcode: 2017PASJ...69...61I

Dotani, Tadayasu; Maeda, Yoshitomo; Mori, Hideyuki +3 more

We analyzed the Suzaku archive data of a type I X-ray burst from GRS 1747-312, a low-mass X-ray binary located in the globular cluster Terzan 6. During the Galactic bulge mapping observations with Suzaku, which covered Terzan 6, an X-ray burst of long duration and with moderate photospheric-radius expansion was serendipitously detected and was con…

2017 Publications of the Astronomical Society of Japan
Suzaku 3
A Galactic Molecular Cloud Clump Catalog from Hi-GAL Data: Method and Initial Results Comparison with BGPS
DOI: 10.3847/1538-4357/835/2/203 Bibcode: 2017ApJ...835..203Z

Rosolowsky, Erik; Zetterlund, Erika; Glenn, Jason

As the precursors to stellar clusters, it is imperative that we understand the distribution and physical properties of dense molecular gas clouds and clumps. Such a study has been done with the ground-based Bolocam Galactic Plane Survey (BGPS). Now the Herschel infrared GALactic plane survey (Hi-GAL) allows us to do the same with higher-quality da…

2017 The Astrophysical Journal
Herschel 3
Retrieval of Venus' cloud parameters from VIRTIS nightside spectra in the latitude band 25°-55°N
DOI: 10.1016/j.pss.2017.06.004 Bibcode: 2017P&SS..144...16M

Piccioni, Giuseppe; Grassi, Davide; Magurno, Davide +2 more

Two years of data from the M-channel of the Visible and InfraRed Thermal Imaging Spectrometer (VIRTIS), on board the European Space Agency mission Venus Express operating around the planet Venus, are analysed. Nocturnal data from a nadir viewpoint in the latitude band 25°N-55°N are selected for their configuration advantages and maximisation of th…

2017 Planetary and Space Science
VenusExpress 3