
|
[az-observing]
||
[Date Prev]
[12-2003 Date Index]
[Date Next]
||
[Thread Prev]
[12-2003 Thread Index]
[Thread Next]
[AZ-Observing] Re: M33's HII Regions
- From: BillFerris@xxxxxxx
- To: az-observing@xxxxxxxxxxxxx
- Date: Mon, 01 Dec 2003 19:12:43 -0500
Jack Jones wrote:
> Your perusal of M33 is most interesting and informative. I was wondering
> what is the easy way to make these arcminute measurements in the field. Do
> you just guesstimate or have a template or reticle in the eyepiece, or use
> a high-power eyepiece with a small known field or what?
In the field, I compare the relative patterns of stars and objects as plotted
on charts, captured in photos/images and presenting at the eyepiece. This
almost always allows me to make a proper ID of an object.
Then later at home, I use MegaStar to determine actual distances and sizes. The
object size estimates are for the apparent size in the eyepice, which is
usually recorded in a sketch. With enough field stars, I can make a
determination that the object--a galaxy for instance--is as "big as the
distance between those two stars" or something like that.
Open star clusters usually appear as large in the eyepiece as they are recorded
in the professional data, unless the outermost members are quite faint. High
surface brightness planetaries often are recorded at their official size or,
perhaps, just a tad bit smaller. Globulars and galaxies often appear
significantly smaller in the eyepiece of my 10-inch than their official sizes
as recorded by the pros. Often, my visual observations record objects between
50% and 75% the official size.
Anyway, getting back to my recent posting on the HII regions in M33, the
distances I used in that posting were determined using MegaStar.
Regards,
Bill Ferris
Flagstaff, Arizona
--
See message header for info on list archives or unsubscribing, and please
send personal replies to the author, not the list.
|

|