Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151

Carole Mundell, A. Pedlar, S. A. Baum, C. P. O'Dea, Jack F. Gallimore, E. Brinks

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The angular resolution of ~0.15 arcsec achieved by MERLIN, is ideal for investigation of neutral gas in the nuclei of nearby Seyferts on scales of less than 10 pc. We present, here, such observations of the radio source associated with the nucleus of NGC 4151. We find that only the component containing the nucleus shows significant absorption, whereas no measurable absorption is seen against other components within the 4 arcsec radio jet. There is structure in the absorption on scales as small as 0.1 arcsec, with column densities in excess of 6x10^21 atoms/cm^2 over parts of the radio nucleus. The neutral hydrogen column densities are much higher than UV absorption measurements which implies that the optical/UV continuum nucleus is not coincident with the strongest radio component. We suggest that the radio nucleus is associated with a weak VLBI component which is ~ 0.1 arcsec (~ 7 pc) to the west of the deepest absorption. We deduce that any neutral hydrogen torus, in which the nucleus is embedded, can be no thicker than 50pc and may have a linear (E- W) extent of less than 40 pc.
Original languageEnglish
Title of host publicationThe XXVIIth Young European Radio Astronomers Conference
EditorsD. A. Green, W. Steffen
Place of PublicationCambridge, U. K.
PublisherCambridge University Press
Publication statusPublished - Mar 1995

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nuclei
hydrogen
very long base interferometry
neutral gases
angular resolution
continuums
atoms

Cite this

Mundell, C., Pedlar, A., Baum, S. A., O'Dea, C. P., Gallimore, J. F., & Brinks, E. (1995). Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151. In D. A. Green, & W. Steffen (Eds.), The XXVIIth Young European Radio Astronomers Conference [21] Cambridge, U. K.: Cambridge University Press.

Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151. / Mundell, Carole; Pedlar, A.; Baum, S. A.; O'Dea, C. P.; Gallimore, Jack F.; Brinks, E.

The XXVIIth Young European Radio Astronomers Conference. ed. / D. A. Green; W. Steffen. Cambridge, U. K. : Cambridge University Press, 1995. 21.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Mundell, C, Pedlar, A, Baum, SA, O'Dea, CP, Gallimore, JF & Brinks, E 1995, Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151. in DA Green & W Steffen (eds), The XXVIIth Young European Radio Astronomers Conference., 21, Cambridge University Press, Cambridge, U. K.
Mundell C, Pedlar A, Baum SA, O'Dea CP, Gallimore JF, Brinks E. Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151. In Green DA, Steffen W, editors, The XXVIIth Young European Radio Astronomers Conference. Cambridge, U. K.: Cambridge University Press. 1995. 21
Mundell, Carole ; Pedlar, A. ; Baum, S. A. ; O'Dea, C. P. ; Gallimore, Jack F. ; Brinks, E. / Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151. The XXVIIth Young European Radio Astronomers Conference. editor / D. A. Green ; W. Steffen. Cambridge, U. K. : Cambridge University Press, 1995.
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abstract = "The angular resolution of ~0.15 arcsec achieved by MERLIN, is ideal for investigation of neutral gas in the nuclei of nearby Seyferts on scales of less than 10 pc. We present, here, such observations of the radio source associated with the nucleus of NGC 4151. We find that only the component containing the nucleus shows significant absorption, whereas no measurable absorption is seen against other components within the 4 arcsec radio jet. There is structure in the absorption on scales as small as 0.1 arcsec, with column densities in excess of 6x10^21 atoms/cm^2 over parts of the radio nucleus. The neutral hydrogen column densities are much higher than UV absorption measurements which implies that the optical/UV continuum nucleus is not coincident with the strongest radio component. We suggest that the radio nucleus is associated with a weak VLBI component which is ~ 0.1 arcsec (~ 7 pc) to the west of the deepest absorption. We deduce that any neutral hydrogen torus, in which the nucleus is embedded, can be no thicker than 50pc and may have a linear (E- W) extent of less than 40 pc.",
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AU - Mundell, Carole

AU - Pedlar, A.

AU - Baum, S. A.

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AU - Gallimore, Jack F.

AU - Brinks, E.

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N2 - The angular resolution of ~0.15 arcsec achieved by MERLIN, is ideal for investigation of neutral gas in the nuclei of nearby Seyferts on scales of less than 10 pc. We present, here, such observations of the radio source associated with the nucleus of NGC 4151. We find that only the component containing the nucleus shows significant absorption, whereas no measurable absorption is seen against other components within the 4 arcsec radio jet. There is structure in the absorption on scales as small as 0.1 arcsec, with column densities in excess of 6x10^21 atoms/cm^2 over parts of the radio nucleus. The neutral hydrogen column densities are much higher than UV absorption measurements which implies that the optical/UV continuum nucleus is not coincident with the strongest radio component. We suggest that the radio nucleus is associated with a weak VLBI component which is ~ 0.1 arcsec (~ 7 pc) to the west of the deepest absorption. We deduce that any neutral hydrogen torus, in which the nucleus is embedded, can be no thicker than 50pc and may have a linear (E- W) extent of less than 40 pc.

AB - The angular resolution of ~0.15 arcsec achieved by MERLIN, is ideal for investigation of neutral gas in the nuclei of nearby Seyferts on scales of less than 10 pc. We present, here, such observations of the radio source associated with the nucleus of NGC 4151. We find that only the component containing the nucleus shows significant absorption, whereas no measurable absorption is seen against other components within the 4 arcsec radio jet. There is structure in the absorption on scales as small as 0.1 arcsec, with column densities in excess of 6x10^21 atoms/cm^2 over parts of the radio nucleus. The neutral hydrogen column densities are much higher than UV absorption measurements which implies that the optical/UV continuum nucleus is not coincident with the strongest radio component. We suggest that the radio nucleus is associated with a weak VLBI component which is ~ 0.1 arcsec (~ 7 pc) to the west of the deepest absorption. We deduce that any neutral hydrogen torus, in which the nucleus is embedded, can be no thicker than 50pc and may have a linear (E- W) extent of less than 40 pc.

M3 - Conference contribution

BT - The XXVIIth Young European Radio Astronomers Conference

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