We propose a 4-epoch PACS photometric monitoring, incoordination with Spitzer and ground-based telescopes,of the newly discovered young eruptive star V2492 Cyg, to verify our hypothesis on rapid re-arrangement ofits circumstellar disk structure.
Publication
Exploring the circumstellar environment of the young eruptive star V2492 Cygni | Kospal A. et al. | Astronomy & Astrophysics Volume 551 id.A62 12 pp. | 551 | 10.1051/0004-6361/201220553 | 2013A&A...551A..62K | http://adsabs.harvard.edu/abs/2013A%26A...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.
European Space Agency, kospal et al., 2012, 'Rapid inner disk re-arrangements in a young eruptive star', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-o05lp57
