Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  15 Cep  ·  22 Cep  ·  22 lam Cep  ·  B173  ·  B174  ·  HD210220  ·  HD210885  ·  HD210905  ·  HD239852  ·  HD239874  ·  HD239923  ·  LBN 482  ·  LBN 485  ·  LBN 486  ·  LBN 489  ·  LBN 490  ·  LBN 491  ·  LDN 1160  ·  LDN 1164  ·  LDN 1165  ·  LDN 1166  ·  LDN 1169  ·  Sh2-134  ·  The star λ Cep
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Sh2 134 (Camera Comparison), Jerry Yesavage
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Sh2 134 (Camera Comparison)

Getting plate-solving status, please wait...
Sh2 134 (Camera Comparison), Jerry Yesavage
Powered byPixInsight

Sh2 134 (Camera Comparison)

Equipment

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Acquisition details

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Description

Repeating one more of the Sharpless2 Group to see what my new CMOS system can find with a deeper look at the H-alpha here..... 

A Previous versions of SH2 134 with more detail of the object itself using 5h on the CCD, but same scope.  Dull by comparison to the 2.5h on the CMOS with the same scope.

Sh2 134 HA RGB


Discussion of GHS aspects of processing:

GHS Forum Discussion

From GalaxyMap:

This HII region is associated with an expanding bubble surrounding Cep OB2. Also associated with this bubble are the HII regions IC 1396 (also called Sh 2-131), Sh 2-129, Sh 2-133, and Sh 2-140.

Avedisova concludes that the 40 solar mass O6 Iab supergiant Lam Cep (HD 210839) is the exciting star for Sh 2-134. You can read about the controversy around the origin of this great Milky Way beacon star in the Cep OB2 section of the Clamshell (110° - 100°) sector portion of the Commentary on the Galactic Plane.

GENERAL NOTE ON SHARPLESS2 OBJECTS>>>>>>>>>>>>>

There are 313 Sh2 objects.  All now imaged.

This is my collection:

Sharpless2

Wide-Angle Hydrogen Alpha Nikon Image Sh2 79-171

Please note there is also a Sharpless2 Group with now more than 2700 examples.

Sharpless2 Group

Other useful links include:

Gary Imm's Collection

GalaxyMap's Collection

The Sharpless Catalog

The MDW H-alpha Sky Survey

Reiner Vogel's detailed observing catalog

Hope you enjoy these obscure but interesting objects...

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