what’s up for imagers the sharpless catalog january 2011 b. waddington

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What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

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Page 1: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

What’s Up for Imagers

The Sharpless Catalog

January 2011

B. Waddington

Page 2: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

It’s Nebula Season Not many galaxies around….. <sigh> But plenty of good nebula opportunities

Larger targets for shorter focal lengths Interesting structure for longer focal lengths Good narrow-band targets |

Page 3: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Hunting Nebula Targets Just as the Arp catalog was a good

resource for finding interesting galaxies… The Sharpless catalog is a great resource

for nebulas Amateur contributions have made this

especially easy to do |

Page 4: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Catalog Developed by Stewart Sharpless at USNO

in late 1950’s Two increments (SH-1, SH-2)

1953 – 142 objects using Palomar Sky survey plates (Baade & Minkowski)

1957 – Final catalog of 313 objects using National Geographic/Palomar Sky Atlas

“Comprehensive” for Dec > -27° |

Page 5: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Catalog Plates taken in both “red” and “blue”; color

used to rule out reflection, planetary nebulas

Catalog included identification of related bright stars

A few “mistakes” – supernova remnants, planetary and reflection nebulas… |

Page 6: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

What Was the Point? Map spatial distribution of hydrogen and

regions of star formation in our galaxy A good tool for building a model of Milky

Way spiral arm structure Also used to refine the galactic pole

position |

Page 7: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Quick Review of “HII regions” HII – ionized hydrogen HI – neutral hydrogen H2 – molecular hydrogen A little bonehead physics:

Atomic Emission Spectra - the Origin of Spectral Lines

|

Page 8: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

HII Region Behavior Nearby bright OB stars ionize the interstellar

hydrogen Free electrons recombine with protons and

release energy (photons) Electrons “cascade” from higher to lower states,

resulting in well-known emission lines The Balmer series emission lines will be the major

components in an amateur image of an emission nebula |

Page 9: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Object Locations

Sharpless RA Values

01020304050607080

Fre

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en

cy

Page 10: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Object Sizes

Sharpless Object Sizes

020406080

100

Diameter, Arc-minutes

Fre

qu

ency

Page 11: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

General Characteristics Wide distribution of sizes, plenty of targets

for all focal lengths Plentiful in Winter and Summer (doh) Good candidates for narrow-band imaging,

especially H-alpha |

Page 12: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Catalog Usage Includes many well-known objects – M42,

Rosette, Lagoon, Cone nebulas… But also provides a path to less well-known

but interesting targets “Shopping” is easy with some excellent

amateur sites |

Page 13: What’s Up for Imagers The Sharpless Catalog January 2011 B. Waddington

Sharpless Resources Dean Salman (“Mr. Sharpless”) :

http://www.sharplesscatalog.com/ Reiner Vogel’s Sharpless Observing Atlas:

http://www.biophysik.uni-freiburg.de/Reiner/ATM/Sharpless/Sharpless_e.html (Sharpless_Atlas.pdf) |