تقرير
The Quasar / Galaxy Pair PKS 1327-206 / ESO 1327-2041: Absorption Associated with a Recent Galaxy Merger
العنوان: | The Quasar / Galaxy Pair PKS 1327-206 / ESO 1327-2041: Absorption Associated with a Recent Galaxy Merger |
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المؤلفون: | Keeney, B. A., Stocke, J. T., Danforth, C. W., Carilli, C. L. |
المصدر: | The Astronomical Journal 141 66 |
سنة النشر: | 2010 |
المجموعة: | Astrophysics |
مصطلحات موضوعية: | Astrophysics - Cosmology and Extragalactic Astrophysics |
الوصف: | We present HST/WFPC2 broadband and ground-based Halpha images, H I 21-cm emission maps, and low-resolution optical spectra of the nearby galaxy ESO 1327-2041, which is located 38 arcsec (14 kpc in projection) west of the quasar PKS 1327-206. Our HST images reveal that ESO 1327-2041 has a complex optical morphology, including an extended spiral arm that was previously classified as a polar ring. Our optical spectra show Halpha emission from several H II regions in this arm located ~5 arcsec from the quasar position (~2 kpc in projection) and our ground-based Halpha images reveal the presence of several additional H II regions in an inclined disk near the galaxy's center. Absorption associated with ESO 1327-2041 is found in H I 21-cm, optical, and near-UV spectra of PKS 1327-206. We find two absorption components at cz = 5255 and 5510 km/s in the H I 21-cm absorption spectrum, which match the velocities of previously discovered metal-line components. We attribute the 5510 km/s absorber to disk gas in the extended spiral arm and the 5255 km/s absorber to high-velocity gas that has been tidally stripped from the disk of ESO 1327-2041. The complexity of the galaxy/absorber relationships for these very nearby H I 21-cm absorbers suggests that the standard view of high redshift damped Lyman-alpha absorbers is oversimplified in many cases. Comment: Replaced with accepted version; 16 pages |
نوع الوثيقة: | Working Paper |
DOI: | 10.1088/0004-6256/141/2/66 |
URL الوصول: | http://arxiv.org/abs/1009.5993 |
رقم الأكسشن: | edsarx.1009.5993 |
قاعدة البيانات: | arXiv |
DOI: | 10.1088/0004-6256/141/2/66 |
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