Detection of Infalling Hydrogen in Transfer between the Interacting Galaxies NGC 5426 and NGC 5427

Using velocity tagging we have detected hydrogen from NGC 5426 falling onto its interacting partner NGC 5427. Our observations, with the GHaFaS Fabry-Perot spectrometer, produced maps of the two galaxies in H Delta *a surface brightness and radial velocity. We found emission with the range of veloci...

Full description

Saved in:
Bibliographic Details
Published in:Astrophysical journal. Letters 2011-10, Vol.740 (1), p.L1-jQuery1323915201739='48'
Main Authors: Font, Joan, Beckman, John E, Rosado, Margarita, Epinat, Benoît, Fathi, Kambiz, Hernandez, Olivier, Carignan, Claude, Gutiérrez, Leonel, Relaño, Monica, Blasco-Herrera, Javier, Fuentes-Carrera, Isaura
Format: Article
Language:English
Subjects:
Arp 271
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BRIGHTNESS
DETECTION
ELEMENTS
EMISSION
GALAXIES
galaxies: individual (NGC 5426
galaxies: interactions
galaxies: ISM
galaxies: kinematics and dynamics
galaxies: spiral
HYDROGEN
INTERACTIONS
LYMAN LINES
MASS
NGC 5427
NONMETALS
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
RADIAL VELOCITY
VELOCITY
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Using velocity tagging we have detected hydrogen from NGC 5426 falling onto its interacting partner NGC 5427. Our observations, with the GHaFaS Fabry-Perot spectrometer, produced maps of the two galaxies in H Delta *a surface brightness and radial velocity. We found emission with the range of velocities associated with NGC 5426 along lines of sight apparently emanating from NGC 5427, superposed on the velocity map of the latter. After excluding instrumental effects we assign the anomalous emission to gas pulled from NGC 5426 during its passage close to NGC 5427. Its distribution, more intense between the arms and just outside the disk of NGC 5427, and weak, or absent, in the arms, suggests that the infalling gas is behind the disk, ionized by Lyman continuum photons escaping from NGC 5427. Modeling this, we estimate the distances of these gas clouds behind the plane: a few hundred parsecs to a few kiloparsecs. We also estimate the mass of the infalling (ionized plus neutral) gas, finding an infall rate of 10 M per year, consistent with the high measured star formation rate across the disk of NGC 5427 and with the detected circumnuclear galactic wind.
ISSN:2041-8205
2041-8213
DOI:10.1088/2041-8205/740/1/L1