Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apj...592..176m&link_type=abstract
The Astrophysical Journal, Volume 592, Issue 1, pp. 176-187.
Astronomy and Astrophysics
Astronomy
2
Ism: Atoms, Ism: Clouds, Ism: Individual: Ngc Number: Ngc 7129, Ism: Reflection Nebulae, Stars: Formation, Stars: Pre-Main-Sequence
Scientific paper
Observations of the environment of the star-forming region NGC 7129 obtained with an angular resolution of 1' in the 21 cm line of H I are described. Two features of the image are extensively discussed: (1) a ring of H I emission about 30' in extent and (2) a relatively dense concentration of H I with unusually wide line profiles positionally coincident with the B star BD +65°1638. The H I ring is consistent with photodissociation of H2 by the interstellar UV radiation field at the surface of an extended molecular cloud in which both BD +65°1638 and NGC 7129 are situated. We further show that BD +65°1638 appears to be an unusual example of a ``dissociating star'' surrounded by an extensive region of photodissociated H2 and accompanied by a small H II region. The derived spectral type (B2.5) and the absolute magnitude for BD +65°1638 further suggest that the latter is very close to the birthline. The very young stellar age implied by the parameters of the H I region, considerably less than 104 yr, is discussed, and the properties of the H I region are compared with those of the prototype for this rare class of objects. We discuss both aspects within the context of star formation in NGC 7129.
Dewdney Peter E.
Matthews Henry E.
Mitchell George F.
Purton C. R.
Roger Robert S.
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