P Cyg

Special Notice #47: Increased Activity in P Cyg

May 19, 2007

P Cyg (2014+37A) is the prototype of massive stars with high mass outflow; it is characterized by blue-shifted emission lines along with red-shifted absorption lines. Surprisingly, we've never created a Variable Star of the Season article for this neat star - I'll have to make sure that happens soon.

Located at

20:17:47.20 +38:01:58.5 J2000

Alert Notice 440: PEP Observing Campaign on P Cygni

Note: This campaign is the subject of the AAVSO Spectroscopy discussion forum thread: https://www.aavso.org/p-cyg-monitoring-intrinsic-h%CE%B1-flux

Also, spectroscopy reports should be submitted to the AAVSO Spectroscopy Database (AVSpec, https://www.aavso.org/apps/avspec/).  -  Elizabeth O. Waagen, 20 May 2020

CONTINUED THROUGH 2021 AT LEAST

P Cygni

P Cygni from the 
Second Digital Sky Survey
A one-degree field of view image of P Cygni, taken from the Second Digital Sky Survey, combining the blue, red, and near-infrared plates in false color (Image courtesy
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