We propose a 4-epoch PACS photometric monitoring, in coordination with Spitzer and ground-based telescopes, of the newly discovered young eruptive star V2492 Cyg, to verify our hypothesis on rapid re-arrangement of its circumstellar disk structure.
Publication
Exploring the circumstellar environment of the young eruptive star V2492 Cygni . Kóspál Á. et al. . Astronomy & Astrophysics, Volume 551, id.A62, 12 pp. . 551 . 10.1051\/0004-6361\/201220553 . 2013A&A...551A..62K ,
Instrument
PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage
2011-10-29T20:44:53Z/2012-01-11T20:08:16Z
Version
SPG v14.2.0
Mission Description
Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.