I’ve been continuing to gather HOYS data as normal and particularly focusing on this star as it’s a bit too low for most people in the evening, but high enough even when below the Pole Star from here in Edinburgh. A lot of the last few weeks data points are mine. Going back to the CCD camera and using real V and R photometric filters has increased accuracy to 0.02 – 0.04 as well.
The star has just undergone a new outburst and is starting to decline again.
The HOYS project reached another recent milestone of 60,00 images in the database. Unfortunately this means the database is now very slow to extract data for lightcurves for. Needs some funding for a developer to work on the database indexing.
A by-product of doing HOYS-CAPS data for V1490Cyg in Tri-colour R, decided to make a stacked image out of it. 30 subs over 6 months.
At least 4 Herbig-Haro objects imaged in this and marked out in the greyscale version.
IC 5070 Pelican Nebula
Cygnus Mag. 8, 60’x50′
250mm f4.8 Newtonian
DSS, Nebulosity, Photoshop
“The Pelican is much studied because it has a particularly active mix of star formation and evolving gas clouds. The light from young energetic stars is slowly transforming cold gas to hot and causing an ionization front gradually to advance outward. Particularly dense filaments of cold gas are seen to still remain, and among these are found two jets emitted from the Herbig–Haro object 555. Millions of years from now this nebula might no longer be known as the Pelican, as the balance and placement of stars and gas will leave something that appears completely different.”
“Herbig–Haro (HH) objects are bright patches of nebulosity associated with newborn stars. They are formed when narrow jets of partially ionized gas ejected by said stars collide with nearby clouds of gas and dust at speeds of several hundred kilometers per second. Herbig–Haro objects are ubiquitous in star-forming regions, and several are often seen around a single star, aligned with its rotational axis. Most of them lie within about one parsec (3.26 light-years) of the source, although some have been observed several parsecs away. HH objects are transient phenomena that last around a few tens of thousands of years. They can change visibly over quite short timescales of a few years as they move rapidly away from their parent star into the gas clouds of interstellar space (the interstellar medium or ISM). Hubble Space Telescope observations have revealed the complex evolution of HH objects over the period of a few years, as parts of the nebula fade while others brighten as they collide with the clumpy material of the interstellar medium.”
Been gathering HOYS-CAPS data on 2MASS J21383981+5708470 in IC1396A recently because of a possible increase in brightness. This has been stretched and processed to show details. Normal submitted data wouldn’t be.
In IC1396A 21 38 39.8 +57 08 47.1
250mm f4.8 Newtonian
Atik 460EX IDAS P2 LP filter Baader tri-colour red filter