CaltechAUTHORS
  A Caltech Library Service

Hubble Space Telescope WFPC2 Imaging of M16: Photoevaporation and Emerging Young Stellar Objects

Hester, J. Jeff and Scowen, Paul A. and Sankrit, Ravi and Lauer, Tod R. and Ajhar, Edward A. and Baum, William A. and Code, Arthur and Currie, Douglas G. and Danielson, G. Edward and Ewald, Shawn P. and Faber, Sandra M. and Grillmair, Carl J. and Groth, Edward J. and Holtzman, Jon A. and Hunter, Deidre A. and Kristian, Jerome and Light, Robert M. and Lynds, C. Roger and Monet, David G. and O'Neill, Earl J., Jr. and Shaya, Edward J. and Seidelmann, Kenneth P. and Westphal, James A. (1996) Hubble Space Telescope WFPC2 Imaging of M16: Photoevaporation and Emerging Young Stellar Objects. Astronomical Journal, 111 (6). pp. 2349-2532. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20150114-085147789

[img] PDF - Published Version
See Usage Policy.

13Mb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20150114-085147789

Abstract

We present Hubble Space Telescope WFPC2 images of elephant trunks in the H II region M16. There are three principle results of this study. First, the morphology and stratified ionization structure of the interface between the dense molecular material and the interior of the H II region is well understood in terms of photoionization of a photoevaporative flow. Photoionization models of an empirical density profile capture the essential features of the observations, including the extremely localized region of [S II] emission at the interface and the observed offset between emission peaks in lower and higher ionization lines. The details of this structure are found to be a sensitive function both of the density profile of the interface and of the shape of the ionizing continuum. Interpretation of the interaction of the photoevaporative flow with gas in the interior of the nebula supports the view that much of the emission from H II regions may arise in such flows. Photoionization of photoevaporative flows may provide a useful paradigm for interpreting a wide range of observations of H II regions. Second, we report the discovery of a population of small cometary globules that are being uncovered as the main bodies of the elephant trunks are dispersed. Several lines of evidence connect these globules to ongoing star formation, including the association of a number of globules with stellar objects seen in IR images of M16 or in the continuum HST images themselves. We refer to these structures as evaporating gaseous globules, or "EGGs." These appear to be the same type of object as the nebular condensations seen previously in M42. The primary difference between the two cases is that in M16 we are seeing the objects from the side, while in M42 the objects are seen more nearly face-on against the backdrop of the ionized face of the molecular cloud. We find that the "evaporating globule" interpretation naturally accounts for the properties of objects in both nebulae, while avoiding serious difficulties with the competing "evaporating disk" model previously applied to the objects in M42. More generally, we find that disk-like structures are relatively rare in either nebula. Third, the data indicate that photoevaporation may have uncovered many EGGs while the stellar objects in them were still accreting mass, thereby freezing the mass distribution of the protostars at an early stage in their evolution. We conclude that the masses of stars in the cluster environment in M16 are generally determined not by the onset of stellar winds, as in more isolated regions of star formation, but rather by disruption of the star forming environment by the nearby O stars.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/117968DOIArticle
http://adsabs.harvard.edu/full/1996AJ....111.2349HADSArticle
ORCID:
AuthorORCID
Grillmair, Carl J.0000-0003-4072-169X
Additional Information:© 1996 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1995 September 21; revised 1996 February 20. It is a pleasure to thank and acknowledge C. F. McKee for a number of interesting comments and suggestions, and in particular for encouraging us to develop here several ideas 2360 originally left for subsequent papers. The authors would also like to thank L. Hillenbrand for making a representation of her IR images available for comparison with the WFPC2 data. Data reductions and analysis were carried out using software running within the IDL environment. This work has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This work was supported by NASA Grant No. NAS-5-1661 to the WF/PC IDT and NASA Contract No. NAS-7-1260 to the WFPC2 IDT. This work was supported at ASU by NASA/JPL contracts 959289 and 959329 and Caltech contract PC 064528.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASANAS-5-1661
NASANAS-7-1260
NASA/JPL959289
NASA/JPL959329
Caltech064528
Issue or Number:6
Record Number:CaltechAUTHORS:20150114-085147789
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150114-085147789
Official Citation:Hubble Space Telescope WFPC2 Imaging of M16: Photoevaporation and Emerging Young Stellar Objects Hester, J. J., Scowen, P. A., Sankrit, R., Lauer, T. R., Ajhar, E. A., Baum, W. A.,, Astronomical Journal v.111, p.2349-2532
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:53670
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Jan 2015 17:55
Last Modified:03 Oct 2019 07:51

Repository Staff Only: item control page