The behavior of the pitch angle of spiral arms depending on optical wavelength
arXiv:1408.5132 · doi:10.1088/2041-8205/793/1/L19
Abstract
Based on integral field spectroscopy data from the CALIFA survey, we investigate the possible dependence of spiral arm pitch angle with optical wavelength. For three of the five studied objects, the pitch angle gradually increases at longer wavelengths. This is not the case for two objects where the pitch angle remains constant. This result is confirmed by the analysis of SDSS data. We discuss the possible physical mechanisms to explain this phenomenon, as well as the implications of the results.
arXiv commentaccepted for publication in ApJ Letters
References in corpus (29)
- Star Formation in Galaxies Along the Hubble Sequence
- The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III
- CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation
- PMAS, the Potsdam Multi-Aperture Spectrophotometer. I. Design, Manufacture, and Performance
- PMAS: The Potsdam Multi Aperture Spectrophotometer. II. The Wide Integral Field Unit PPak
- CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release
- Self-Perpetuating Spiral Arms in Disk Galaxies
- Dynamics of Non-Steady Spiral Arms in Disk Galaxies
- On the origin of rR_1 ring structures in barred galaxies
- Rings and spirals in barred galaxies. I Building blocks
- Measurement of Galactic Logarithmic Spiral Arm Pitch Angle Using Two-Dimensional Fast Fourier Transform Decomposition
- Discovery of a relationship between spiral arm morphology and supermassive black hole mass in disk galaxies
- Rings and spirals in barred galaxies. III. Further comparisons and links to observations
- Constraining corotation from shocks in tightly-wound spiral galaxies
- The Lifetimes of Spiral Patterns in Disc Galaxies
- Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. I. Method outline
- On the galaxy spiral arms' nature as revealed by rotation frequencies
- Spiral density wave triggering of star formation in SA and SAB galaxies
- The Onset of Spiral Structure in the Universe
- A test of arm-induced star formation in spiral galaxies from near-IR and H imaging
- Further Evidence for a Supermassive Black Hole Mass - Pitch Angle Relation
- Tracing the Dynamics of Disk Galaxies with Optical and IR Surface Photometry: Color Gradients in M99
- Pitch angle variations in spiral galaxies
- Gaseous Spiral Structure and Mass Drift in Spiral Galaxies
- The coalescence of invariant manifolds and the spiral structure of barred galaxies
- Signatures of long-lived spiral patterns
- Testing theories in barred spiral galaxies
- PINGSoft: an IDL visualisation and manipulation tool for Integral Field Spectroscopic data
- The shock-induced star formation sequence resulting from a constant spiral pattern speed
Cited by in corpus (15)
- CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release
- CALIFA, the Calar Alto Legacy Integral Field Area survey. III. Second public data release
- Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges
- The shapes of spiral arms in the SG survey and their connection with stellar bars
- Dependence of Spiral Arms Pitch Angle on Wavelength as a Test of Density Wave Theory
- On the Connection Between Spiral Arm Pitch Angle and Galaxy Properties
- Strong Evidence for the Density-wave Theory of Spiral Structure in Disk Galaxies
- The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations
- Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study
- Strong spiral arms drive secular growth of pseudo bulges in disk galaxies
- Searching for Intermediate Mass Black Holes in galaxies with Low Luminosity AGN: A multiple-method approach
- Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Colour jumps across the spiral arms of Hubble Ultra Deep Field galaxies
- SpArcFiRe: morphological selection effects due to reduced visibility of tightly winding arms in distant spiral galaxies