Complutense University Library

Long-slit spectroscopy and direct imaging of the PMS objects GGD-33 and V-350 cephei in NGC-7129

Miranda, L. F. and Gómez de Castro, Ana Inés and Eiroa, C. and Fernández, M. (1994) Long-slit spectroscopy and direct imaging of the PMS objects GGD-33 and V-350 cephei in NGC-7129. Astronomy & Astrophysics, 281 (3). pp. 864-870. ISSN 0004-6361

[img] PDF
Restricted to Repository staff only until 31 December 2020.

179kB

Official URL: http://adsabs.harvard.edu/abs/1994A&A...281..864M

View download statistics for this eprint

==>>> Export to other formats

Abstract

We present CCD images and long-slit spectra of the nebulous object GGD 33 and of the T Tauri star V 350 Cep in the star formation region NGC 7129. The data suggest that GGD 33a is a T Tauri star and likely the illuminating source of the whole GGD 33. Evidence of variability of GGD 33a is presented. Double-peaked [S II] emission lines are observed in GGD 33a. The high-velocity component of the [S II] emission could be related to a HH jet-like outflow observed very close to the star. V 350 Cep is embedded in a reflection nebulosity. High velocity mass outflow, detected through its blueshifted Halpha emission, seems to emanate from V 350 Cep. The spectrum of V 350 Cep presents a large number of permitted emission lines, but, except [S II], no forbidden emission lines have been identified in our spectra.


Item Type:Article
Uncontrolled Keywords:Herbig-haro objects; t-tauri stars; emission-line; optical jets; young stars; outflows; region; Stars, pre-main-sequence; stars, individual, v-350 cep; ism, individual objects, ngc-7129, ggd-33 (in ngc-7129); ism, jets and outflows
Subjects:Sciences > Mathematics > Astronomy
ID Code:16551
Deposited On:27 Sep 2012 08:33
Last Modified:27 Sep 2012 08:33

Repository Staff Only: item control page