Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk

A. Müller; M. Keppler; Th. Henning; M. Samland; G. Chauvin; H. Beust; A.-L. Maire; K. Molaverdikhani; R. van Boekel; M. Benisty; A. Boccaletti; M. Bonnefoy; F. Cantalloube; B. Charnay; J.-L. Baudino; M. Gennaro; Z. C. Long; A. Cheetham; S. Desidera; M. Feldt; T. Fusco; J. Girard; R. Gratton; J. Hagelberg; M. Janson; A.-M. Lagrange; M. Langlois; C. Lazzoni; R. Ligi; F. Ménard; D. Mesa; M. Meyer; P. Mollière; C. Mordasini; T. Moulin; A. Pavlov; N. Pawellek; S. P. Quanz; J. Ramos; D. Rouan; E. Sissa; E. Stadler; A. Vigan; Z. Wahhaj; L. Weber; A. Zurlo

doi:10.1051/0004-6361/201833584

Home

All issues

Volume 617 (September 2018)

A&A, 617 (2018) L2

Full HTML

Free Access

Fig. B.1.

Open with DEXTER Download original image

IRDIS combined K₁K₂ image of PDS 70 using classical ADI. To increase the dynamic range of the faint disk structures, the companion’s full intensity range is not shown. The black lines indicate the structures discussed in the above text. North is up, east is to the left.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.