Bibcode
GRAVITY Collaboration; Abuter, R.; Accardo, M.; Adler, T.; Amorim, A.; Anugu, N.; Ávila, G.; Bauböck, M.; Benisty, M.; Berger, J. -P.; Bestenlehner, J. M.; Beust, H.; Blind, N.; Bonnefoy, M.; Bonnet, H.; Bourget, P.; Bouvier, J.; Brandner, W.; Brast, R.; Buron, A.; Burtscher, L.; Cantalloube, F.; Caratti O Garatti, A.; Caselli, P.; Cassaing, F.; Chapron, F.; Charnay, B.; Choquet, É.; Clénet, Y.; Collin, C.; Coudé Du Foresto, V.; Davies, R.; Deen, C.; Delplancke-Ströbele, F.; Dembet, R.; Derie, F.; de Wit, W. -J.; Dexter, J.; de Zeeuw, T.; Dougados, C.; Dubus, G.; Duvert, G.; Ebert, M.; Eckart, A.; Eisenhauer, F.; Esselborn, M.; Eupen, F.; Fédou, P.; Ferreira, M. C.; Finger, G.; Förster Schreiber, N. M.; Gao, F.; García Dabó, C. E.; Garcia Lopez, R.; Garcia, P. J. V.; Gendron, É.; Genzel, R.; Gerhard, O.; Gil, J. P.; Gillessen, S.; Gonté, F.; Gordo, P.; Gratadour, D.; Greenbaum, A.; Grellmann, R.; Grözinger, U.; Guajardo, P.; Guieu, S.; Habibi, M.; Haguenauer, P.; Hans, O.; Haubois, X.; Haug, M.; Haußmann, F.; Henning, T.; Hippler, S.; Hönig, S. F.; Horrobin, M.; Huber, A.; Hubert, Z.; Hubin, N.; Hummel, C. A.; Jakob, G.; Janssen, A.; Jimenez Rosales, A.; Jochum, L.; Jocou, L.; Kammerer, J.; Karl, M.; Kaufer, A.; Kellner, S.; Kendrew, S.; Kern, L.; Kervella, P.; Kiekebusch, M.; Kishimoto, M.; Klarmann, L.; Klein, R.; Köhler, R.; Kok, Y. et al.
Bibliographical reference
The Messenger
Advertised on:
12
2019
Citations
0
Refereed citations
0
Description
Near-infrared interferometry gives us the opportunity to spatially resolve the circumstellar environment of young stars at sub-astronomical-unit (au) scales, which a standalone telescope could not reach. In particular, the sensitivity of GRAVITY on the VLTI allows us to spatially resolve the CO overtone emission at 2.3 microns. In this article, we present a new method of using the model of the CO spectrum to reconstruct the differential phase signal and extract the geometry and size of the emitting region.