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INTRIGUING HERBIG OBJECTS

More than just proto disks, close inspection reveals much more, for instance   junior   and the Sirian cousins

Go to spiky Lkha 233
Go to Lkha 198 and juvenile
Go to Lkha 198-IR with spike

Go to tidal trios at nearby giant star Beta Cassiopeiae
Go to anomalies at large star Epsilon Bootis
Go to anomaly at large star Beta Pictorus

Go to two bojangles at Sirius
Go to star 51 Pegasi - solar huff and puff, brown dwarf nearby, gravitic striations

HERBIG   AE/BE   STARS LKHA 198   and   LKHA 233

Link for Lkh-alpha 198 and Lkh-alpha 233 information - two Herbig Ae/Be class new stars (mass range 1.5 to 10 times our Sun mass) with proto forms involved

LKHA 198

There is no escaping the presence of a juvenile proto (dark) which, if a large star, has not yet turned on, if an exotic kind of star, is silent. The juvenile proto is roughly the same size and shape as Lkha 198 (bright)



The real Junior is in the upper left. A dark dot with tail is seen at the right edge, midscreen

In the above composite, a copy of dark junior has been moved and rotated alongside bright Lkha 198 for easy comparision. Junior inserted beside Lkha 198 makes details in junior more saliently seen, for instance the round upper end inside junior's crescent yin-yang could be the outline of a proto star density, the outlining edge is roughly of similar size to the star already aglow in Lkha 198

As a matter of fact, in viewing the above composite in 3d (merge the two images together by eyesight) the broad latticed arc in the middle of junior may be a disk segment set at sharp angle declenting from the outer dark proto disk, which means a possibility that a silent object with strong gravity is inside the broad arc in the middle of junior

Four views next each reveal subtle differences, the combination of four images are the 'view'. Associated Herbig object Lkha 198-ir is the smaller star nearby with a bent toggle sticking out









In the bright view immediately above, in 3d - (focus the two images together by eyesight) - the white oval ring is seen entering a vertical collar immediately to the left of the star, the point of entry is farther away in the oval's tilt, therefore farther from the camera. Indications are enough to suggest the upper left end of the white rim is diving into a small vertical disk which is immediately to the left of the big star. There is enough going on to suggest at least one silent partner star may be involved in the system

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The bright oval disk structure enhanced with histogram to blur its details and distinctify its fundamental outlines, which is similar to the juvenile, which makes the juvenile a member of the family, not a spurious fault in the photo


Noticable, is that the juvenile is a reverse negative to the adult, that is, where the adult's crescent is light, the juvenile's crescent is dark, and where the juvenile's thick rightside outflank is light, the adult's rightside thick outflank is dark



Original - dark with dim oval - no trace of junior






Gamma enhanced - junior is easily seen with gamma correction amplifying resident dim media in the image



Left, a view more starkly outlined by use of other image adjusters - which indicate (but image weakness does not prove) more than one secondary small rings are at different angles attached to the main oval.

In the small side by side pair above, a tiny dark dot with tail is similar to proplyds seen at Orion in trapezium photos by Hubble - the tiny dot here it too small to enlarge or pull closer by more than a modicum of zoom, you are looking at the modicum

Shadowed dots are seen in Dss plates every so often, this modicum above is shown because it is easy to see. Shadow dots like this would be expected to have tails away from a bright object (like an eclipse penumbra shadow) but penumbra tails do not seem to be a rule. Giant star Beta Cassiopeiae is to the upper right offscreen, for example, and the shadow tail in the modicum is not pointing away from it, rather, toward it but vectored well to the left of Cassiopeiae, the tail is not a penumbra shadow of Cassiopeiae





Large new star Lkh-apha 198, also Lkha 198, with a proto disk, which may not be a simple one-purpose proto disk in that two small white stars are easily seen and seem located in the oval rim, the big star itself is strongly displaced regards the oval, and there is a peculiar small dot or star inside the oval, peculiar because this small 'star' does not enlarge or change size under strong enhancements (which otherwise invariably enlarge bright objects in spurious ways)





Two bright small light points are on the rim of the oval, one across from the other. Inside the oval at roughly the focii of one end of an ellipse, a very tiny light point does not noticably change size when the image is highly enhanced, this is unusual, usually stars swell absurdly in size when absurd quantities of image enhancements are applied. It cannot be said with certainty (in the limits of this Dss image), if, or if not, the two bright dots in the oval rim are chance overlays from afar, not embodied in the rim

LKHA 198-IR WITH SPIKE



Object Lkha 198-IR (little guy with toggle) is nearby but not neccessarily a neighbor, with a small jet curling to the right

Different enhancements seen further above, do not support a jet with 100% certainty, the 'jet' may be a portion of disk aglow, but seems more a chance occurance of spurious nature as drifting Lkha 198-ir temporarily excites a small but dense matter waft of sundry nature (of course, spectroscopies will tell at once if the bright toggle is a high energy jet, a disk lit up, or external excitement of a passing low energy waft)

Lkha 198 is in proximity to the field view of large star Beta Cassiopeiae, the location of Lkha 198 is by coincidence in sight of the large star, it is not in the star's solar family

Click for expanded to scale
Click for larger field view



At left is a garrish plate error in the Dss Poss1 infrared plate for Beta Cassiopeiae. Click for larger field image. This is an obvious belly button lint flaw, it is stark without glow or other fundamentals around it

Flipping the coin, objects with any glow I tend to regard as artifacts of astronomy rather than flaws of photography. Objects such as these (image far left - and located further above to the right in the same plate) I tend to regard as good positives, worth a second look to verify if false or not

The Dss Poss1 A plate for Beta Cassiopeiae reveals at least three tidal trios in the star's solar family, the image density is dim the trios are not easily seen even under high enhancement

Click for large image



In the Dss Poss1 red plate at least one tidal trio is visible, plus noticable quantities of guff (of a kind expected from powerful coronal mass ejections) crowd the inner region near the surface of the star

Finished - Lkha 198

AT SIRIUS - TWO BOJANGLES

Super star Sirius has two bojangles in orbit in its solar field, the two have a look and feel enough to be possible cousins of junior, in which case two possible Herbig class objects (or lower mass relatives) are in an orbit around Sirius



Sirius is huge, a touch of its hem (an arc of about 15 percent) is in the upper right when you click the image for large

Click for large showing Sirius



These two tidal objects (in company with two tidal trios), have been called 'commas' in the Trios.htm page

HERBIG AE/BE OBJECT LKHA 233

Dss original



Enhanced, showing complex organization





There is talk in town that jets are seen at Lkha 233. Enhancement can suggest that the north/west and south/east fingers are chance overlay revealing an illuminated arcing thin strip of excited matter detached from the star, discontinuities close to the star can be see in the 'jets', suggesting alternative interpretations other than jets

The star (and jet whatevers) are otherwise obviously attached to a larger structured organization immediately to the east of the star, the structuring includes vertical diskal forms dimly brought out in strong image enhancings

The region of space itself has drifts in bands, the drifts are far to dim to be coaxed into clear view by normal image adjusters. Histrogram produces views that are two grainy and diffuse and so are of little use also. However, the Dpi of a graphic editor's thumbnail browser is particularly high, and this (thumbnail Dpi) reveals that Herbig item Lkha 233 is actually in a rather intertersting conflux. The next tableau view shows 4 different histogram renderings of different Dss plates, plus a plate in which tiny Lkha 233 is shown in a color square in the leftmost thumbnail



Two strong strands meander across the screen, in the middle a large diffusive surge comes forward over which is spilling a tongue, within which is Lkha 233. From the middle of the surge, on its east side, a strong strand exits continuing east, in other words the strand is the stronger life form (ahem) sustaining its strand bandwidth passing inside through the surge. These (in Cosmicastronomy.com) are the first images shown revealing where strong bands are crisscrossing through a conjuctive nexus where Lkha 233 has formed as a large new star



LARGE DOTS

Large dots are found in a Dss plate featuring Herbig Ae/Be object Lkha 233, these dots could be large enough to comprise bodies in a size range from extra large gas planets, to small underline stars too feeble for nuclear processes to kick in. Some noticable large dark spots in the Lkha 233 region, seen in the Poss2 Dss plate. A small object in greytone at the bottom left (click on image for large) does not have an immediate interpretation

Click for large color version
Click Click for large histogram version





The Dss Poss1 infrared plate for Lkha 233 is peppered with dark dots

Click for full size view of small dark dots



Dark dots of various mishappen kind, and in clusters, and small diffuse dark dots, are everywhere in the Dss Poss1 infrared plate. It can be felt that these dark dots are planets, it can also be felt that these dark dots are errors in the plate, the felt sense is strongest in favor of planets scattered everywhere, which suggests areas of space may be filled with rogue wandering planets which do not have orbits, but...

Finished - Lkha 233

LARGE STAR EPSILON BOOTIS

At Epsilon Bootis

Epsilon Bootis earns its price of admission in an infrared Dss Poss1 plate which contains a spheroid with dark center unlike anything seen elsewhere so far by astronomy anomaly spotters, about the closest proximity to a description is a large planet with huge outer mass shell and inner (dark) ellipsical planetoid disk large enough to hide the planet

The very strange anomalous object is easily noticed at Epsilon Bootis

Very dim (hardly detectable) in the original (at left), plainly visible in photo enhancement (right image)

The round object does not enhance well via various image adjusters available in home kitchen table style Pc graphic editors. Three different enhanced views (the second pair can be seen in 3d by using eyesight to focus the two views together) are shown to reveal the anomolous object in different styles, giving different ways to appreciate it

The object is an apparent spheroid formation however its internal ingrediants, and density tones, do not match any other object seen in a large survey of Dss plates comprising dozens of different large and giant stars, whose anomalies include flyers, aka tidal trios, and possible brown dwarf stars

Next, the anomalous object in context of the greater star region, (Dss Poss1 infrared - object is in upper right corner). Flotsum and jetsum is floating around the star's solar wind halo

Click for large image



At Epsilon Bootis - tidal trio

A strong tidal trio made of simple ovals. Other dim ovals are hording around the giant star

Click for large image



This tidal trio is seen at Epilon Bootis, standing out noticably in regional solar space crowded with miscellaneous ovals

This giant star (Epsilon Bootis - where some ufo wingnuts believe is the homeworld of an alien probe in an Earth-moon trojan orbit for 12,000 years), is lopsided, more of its outer halo brillience is strongly biased in a north/east diffuse outbulge seen in red filters. The outbulge is south/west in the infrared Poss1 plate. The outbulge is seen is these following Dss high Dpi thumbnail views of Epsilon Bootis

Epsilon Bootis is not pictured in perfectly spherical form, histogram views of Dss Poss1 red plate (left) and Poss1 infrared plate (far left) show mass density irregularities and drifts predominating the star, the two different energy plates show two distinctly different densities


A thin pinworm (colorized view left) is in the Dss Poss2 infrared plate. Also, an indistinct white object (image far left)

The thin pinworm does not have the hard dark outlines of a plate flaw, the string is tagged to a tiny dim oval of unknown nature, in toto this may be a string of denser proto matter, probably not long lasting as a pinworm string, it may in fact be the result of an astronomer's sneeze

AT BETA PICTORUS - ANOMALOUS STRANGE OBJECT



An anomalous strange object with a cannister outline is floating in the field plate of Beta Pictorus, the object seems to have stereo components therefore (if a 3D form) is not a plate flaw which would be entirely flat despite being viewed in 3D



51 PEGASI

At 51 Pegasi - a strange quilt patch floating in the solar wind





The large patch is in parallel checkerboards with vertical arc components. The parallels do not vector to the star. Is it possible this is a stray clump drifting by, it is only seen in the Dss Poss1 infrared plate no trace is seen in any other Dss plate for 51 Pegasi, so the patch is either a frequency thing, or an eyeblink in time chance event

At 51 Pegasi - a large dark hole

Possible candidate as a brown dwarf star, the dark hole is seen only in the Dss Poss1 infrared plate, which means the dark hole glows with only dull heat





The dark hole is not visible at all in the plate original. Histogram reveals the dark hole at once



At 51 Pegasi - gravitic striations



The ripples (gravity waves) are extremely dim, seen only in the Dss Poss2 red plate. Histogram shows them at once. High levels of illumination adjustment reveals them against a grey backdrop of deep space

A faint outer ring surrounds 51 Pegasi



Note: gravitic striations are a big topic in Cosmicastronomy.com. A recent addition is an exploration of a major gravitic sea surrounding giant star Epsilon Cma

The main thunbnail page for gravity waves is Edge.htm

Related sites
Planets.htm     Planets1.htm     Planets2.htm     Hark.htm     Trios.htm     Flyers.htm     Regulus.htm     Rilldisk.htm     Ringling.htm     Darkhole.htm     Dwarfs.htm    

Web site/display/designs/image enhancements - Greydon Moore World's largest cosmic teaching site - Ottawa 2001/2004         form   A & O 3 3