Hostname: page-component-54dcc4c588-dbm8p Total loading time: 0 Render date: 2025-10-07T15:40:37.328Z Has data issue: false hasContentIssue false

Exploring Planetary Nebulae in the dwarf galaxy VCC 1249 using MUSE data

Published online by Cambridge University Press:  06 October 2025

Sophie Penger*
Affiliation:
University of Cologne, Germany, European Southern Observatory, Germany, Finnish Centre for Astronomy with ESO (FINCA), Finland, Waterloo Centre for Astrophysics, Canada
Johanna Hartke
Affiliation:
University of Cologne, Germany, European Southern Observatory, Germany, Finnish Centre for Astronomy with ESO (FINCA), Finland, Waterloo Centre for Astrophysics, Canada
Magda Arnaboldi
Affiliation:
University of Cologne, Germany, European Southern Observatory, Germany, Finnish Centre for Astronomy with ESO (FINCA), Finland, Waterloo Centre for Astrophysics, Canada
Ana Inés Ennis
Affiliation:
University of Cologne, Germany, European Southern Observatory, Germany, Finnish Centre for Astronomy with ESO (FINCA), Finland, Waterloo Centre for Astrophysics, Canada

Abstract

This study focuses on investigating planetary nebulae (PNe) within the dwarf galaxy VCC 1249, located in the halo of the early-type galaxy (ETG) M49, by utilizing data obtained from the Multi-Unit Spectroscopic Explorer (MUSE). The integral-field spectroscopy capabilities of MUSE enable the identification of individual planetary nebulae. The interaction of VCC 1249 with the cluster-dominant galaxy M49 in the Virgo Subcluster B is driving this project, as it offers a unique opportunity to explore how high-density environments influence the properties and fate of low-mass galaxies. To identify potential PNe candidates within VCC 1249, the method proposed by Roth et al. (2021) is employed. Through this approach, ten candidates exhibiting features consistent with PNe properties have been identified.

Information

Type
Poster Paper
Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable

References

Arrigoni Battaia, F., Gavazzi, G., Fumagalli, M., et al. 2012, A&A, 543, A112 Google Scholar
Bacon, R., Accardo, M., Adjali, L., et al. 2010, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol. 7735, Ground-based and Airborne Instrumentation for Astronomy III, ed. McLean, I. S., Ramsay, S. K., & Takami, H., 773508Google Scholar
Ciardullo, R., Feldmeier, J. J., Jacoby, G. H., et al. 2002, ApJ, 577, 31 CrossRefGoogle Scholar
Errani, R., Penarrubia, J., & Tormen, G. 2015, MNRAS, 449, L46 CrossRefGoogle Scholar
Ferrarese, L., Côté, P., Cuillandre, J.-C., et al. 2012, ApJS, 200, 4 CrossRefGoogle Scholar
Hartke, J., Arnaboldi, M., Gerhard, O., et al. 2018, A&A, 616, A123 Google Scholar
Peñarrubia, J., Benson, A. J., Walker, M. G., et al. 2010, MNRAS, 406, 1290 Google Scholar
Roth, M. M., Jacoby, G. H., Ciardullo, R., et al. 2021, ApJ, 916, 21 CrossRefGoogle Scholar
Supplementary material: File

Penger et al. supplementary material

Penger et al. supplementary material
Download Penger et al. supplementary material(File)
File 890.8 KB