Studies of Resolved Objects in M31



July 24, 2009, rev 2

This page contains a description of an on-going study of star clusters, HII regions, PNe and individual stars in M31 done with Hectospec on the MMT by Nelson Caldwell and a host of others1.  The first paper of the project has been published:
Star Clusters in M31: I. A Catalog and a Study of the Young Clusters (AJ, 2009, 137, 94).

At this web site, you will find the new M31 cluster catalog and links to the ground based and HST images of stars and clusters.  Also appearing are the spectra of the young clusters and individual stars .  Spectra and velocities of the old clusters will be released upon acceptance of that paper.

Ideally, this site would be a WIKI site, but currently the CfA doesn't allow such sites. If anyone else has ideas about how and where to create such  a site, I'd be delighted to help out with that.

Regards,

caldwell here at cfa.harvard.edu


1Including but not limited to : Heather Morrison, Paul Harding, Jim Rose, Ricardo Schiavon, Genevieve Graves, Jeff Kreissler, Jay Strader.


Images of Clusters and Stars in the revised Hectospec M31 catalog

Spectra and Images of just Star Clusters in M31

Images of Old Star Clusters in M31, ordered by estimated mass

Spectra and Images of Young Star Clusters in M31, ordered by estimated mass

Spectra and Images of Young Star Clusters in M31, ordered by estimated age

Images and Spectra of Stars in the M31 catalog



Spectra


Spectra of the young clusters and the stars are now available at the links above. These are in jpg format currently. Click on the postage stamp for full resolution. The spectra (aside of a few problem cases that are obvious - young clusters with red continua) have been flux calibrated, deredshifted (actually deblueshifted) and dereddened. These plots show only the blue part of the spectrum. The data was smoothed before plotting. At a later time I will make the actual spectra available. Spectra do exist for most of the old clusters, but won't be released till that paper is published.

Postage stamp images of selected Objects in M31


These images come from three sources: the digitized Palomar survey, the Local Group Survey of Massey et al. 2006, AJ, 131, 2478, and HST (ACS or WFPC2). For each object in these lists, the following are shown:
The HST images are not complete, and in some cases what is shown is merely one image out of a sequence, because the HST archive hasn't yet combined those images.  Those will contain annoying cosmic ray hits.  Each web page contains a list of objects to the left, ordered as stated. The images will appear to the right after clicking. The names used are those from the RBC, and basic information appears next to the images (type, velocity, V magnitude, comments).  "Type" is explained in the catalog notes (see link below).

The WCS on the HST images is not always good, so sometimes the target will be offcenter in the HST images. The images all have N at the top, East to the left (which isn't true for the images in the paper - oops!).

I have made great use of these images to clean up the cluster catalog, but that job is not complete - every day or so I change an object's classification from cluster to star or vice-versa.  If anyone else takes the time to look through these and notes a discrepant type, please feel free to advise me so that I can make changes to the catalog.

Note that objects with an "x" suffix were initially thought to be the object (usually the real object is a few arcsecs away and more difficult to see), and were observed with Hectospec before the mistake was realized. These are nearly all stars.


AAS machine format for the catalog

I don't actually use this format myself, preferring starbase format (tab delimited), but anyway, here is the entire Hectospec catalog, ordered by RA, and containing the updated coordinates,  V magnitudes where extant, a rough type classification, and some notes as described in the table and the paper.  This catalog includes more objects than are in the catalog paper, and is believed to incorporate all the Revised Bologna catalog (Galleti et al. 2007, A&A, 471, 127) entries  except for a handful of the clusters found on HST images and reported in the papers of Hodge and collaborators. Eventually those will appear here as well.   Several hundred entries labeled "bstar", "astar", "fstar", or "ysg" (yellow supergiant) are also included, and can safely be ignored for the time being.  The type classification comes mostly from the spectra, though for a few cases where I don't have spectra but the images (or previous detailed work) indicate an old cluster, I say that.

This version is more up-to-date than the published version contained in the aforementioned paper.

M31 Hectospec catalog

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