Query : 2013A&A...551A..81V

2013A&A...551A..81V - Astronomy and Astrophysics, volume 551A, 81-81 (2013/3-1)

How does star formation proceed in the circumnuclear starburst ring of NGC 6951 ?


Abstract (from CDS):

Gas inflowing along stellar bars is often stalled at the location of circumnuclear rings, which form an effective reservoir for massive star formation and thus shape the central regions of galaxies. However, how exactly star formation proceeds within these circumnuclear starburst rings is the subject of debate. Two main scenarios for this process have been put forward. In the first, the onset of star formation is regulated by the total amount of gas present in the ring with star forming starting, once a mass threshold has been reached, in ``random'' positions within the ring like ``popcorn''. In the second, star formation primarily takes place near the locations where the gas enters the ring. This scenario has been dubbed ``pearls-on-a-string''. Here we combine new optical IFU data covering the full stellar bar with existing multiwavelength data to study the 580pc radius circumnuclear starburst ring in detail in the nearby spiral galaxy NGC6951. Using Hubble Space Telescope (HST) archival data together with SAURON and OASIS IFU data, we derive the ages and stellar masses of star clusters, as well as the total stellar content of the central region. Adding information on the molecular gas distribution, stellar and gaseous dynamics, and extinction, we find that the circumnuclear ring in NGC6951 is ∼1-1.5Gyr old and has been forming stars for most of that time. We see evidence for preferred sites of star formation within the ring, consistent with the ``pearls-on-a-string'' scenario, when focusing on the youngest stellar populations. The ring's longevity means that this signature is washed out when older stellar populations are included in the analysis.

Abstract Copyright:

Journal keyword(s): galaxies: individual: NGC 6951 - galaxies: ISM - galaxies: stellar content

VizieR on-line data: <Available at CDS (J/A+A/551/A81): list.dat maps/* table4.dat table5.dat>

Nomenclature: Tables 4-5: [VSE2013] NN (Nos 1-55).

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 2

goto Full paper

goto View the references in ADS

Number of rows : 2
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
1 NGC 1097 LIN 02 46 19.059 -30 16 29.68 10.46 9.97 9.48 8.72 9.8 ~ 1263 3
2 NGC 6951 Sy2 20 37 14.1228088488 +66 06 20.049916392   11.64 10.65     ~ 512 2

To bookmark this query, right click on this link: simbad:objects in 2013A&A...551A..81V and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact