First ultra-compact dwarf galaxy in the group NGC 5044 found

February 27, 2017 by Tomasz Nowakowski report
This image shows a composite view of the giant elliptical galaxy NGC 5044. Credit: Digitised Sky Survey/NASA Chandra/Southern Observatory for Astrophysical Research/Very Large Array (Robert Dunn et al. 2010)

(Phys.org)—A team of astronomers led by Favio Faifer of the National University of La Plata, Argentina, has discovered the first ultra-compact dwarf (UCD) galaxy in an X-ray bright galaxy group designated NGC 5044. The finding was presented Feb. 21 in a paper published online on the arXiv pre-print repository.

Located some 116 million light years away, NGC 5044 is an early-type massive elliptical galaxy residing at the center of an X-ray bright group also named NGC 5044. This group contains about 150 members, most of which are dwarf galaxies. Although the group's center galaxy has been the subject of several past studies, its globular cluster and UCD system remain unexplored.

UCDs are very compact galaxies with high stellar populations, containing about 100 million stars. They display masses, colors, and metallicities between those of and early-type dwarf galaxies. These ultra-compact stellar systems could provide important insights on the formation and evolution of galaxies in the universe.

That is why Faifer's team observed the NGC 5044 with the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope in Chile. They obtained deep images of several fields around NGC 5044, which allowed them to detect the presence of a UCD.

"From the photometric and spectroscopic analysis of a deep field taken with Gemini+GMOS, we have been able to detect and confirm the first UCD in the NGC 5044 group," the researchers wrote in the paper.

The radial velocity and angular proximity (2.83 arcmin) of this UCD indicate that this object is associated with galaxy NGC 5044. The newly discovered UCD was designated NGC 5044-UCD1.

The researchers found that the metallicity of NGC 5044-UCD1 is within the range displayed by other UCD detected in constellations Virgo and Fornax, but considerably lower than that of the confirmed stripped nuclei described in previous studies. They also studied the star formation history of this UCD and found that this object is approximately 11.7 billion years old.

Although the origin of UCDs is still widely debated, the most plausible hypotheses suggest that they are massive star clusters or the nuclei of tidally stripped . The scientists assume that NGC 5044-UCD1 could be such an unusually massive globular cluster. They note that the object's luminosity is well above the usual upper cut for "classical" globular clusters. Furthermore, NGC 5044-UCD1 presents a supersolar α-element abundance of [α/Fe] = 0.30, suggesting rapid star formation, typical for most globular clusters.

"All the lines of evidence would point toward NGC 5044-UCD1 being an unusually massive globular cluster of the NGC 5044 system," the paper reads.

Further spectroscopic observations could reveal more insights on the true nature of NGC 5044-UCD1. Currently, the team prepares an analysis of the complete photometric dataset, what will be presented in a forthcoming paper.

Explore further: Image: Hot gas sloshing in a galactic cauldron

More information: First confirmed ultra-compact dwarf galaxy in the NGC 5044 group, arXiv:1702.06472 [astro-ph.GA] arxiv.org/abs/1702.06472

Abstract
Context. Ultra-compact dwarfs (UCDs) are stellar systems displaying colours and metallicities between those of globular clusters (GCs) and early-type dwarf galaxies, as well as sizes of Reff <= 100 pc and luminosities in the range -13.5 < MV < -11 mag. Although their origin is still subject of debate, the most popular scenarios suggest that they are massive star clusters or the nuclei of tidally stripped dwarf galaxies. Aims. NGC 5044 is the central massive elliptical galaxy of the NGC 5044 group. Its GC/UCD system is completely unexplored. Methods. In Gemini+GMOS deep images of several fields around NGC 5044 and in spectroscopic multi-object data of one of these fields, we detected an unresolved source with g'~20.6 mag, compatible with being an UCD. Its radial velocity was obtained with FXCOR and the penalized pixel-fitting (pPXF) code. To study its stellar population content, we measured the Lick/IDS indices and compared them with predictions of single stellar population models, and we used the full spectral fitting technique. Results. The spectroscopic analysis of the UCD revealed a radial velocity that agrees with the velocity of the elliptical galaxy NGC 5044. From the Lick/IDS indices, we have obtained a luminosity-weighted age and metallicity of 11.7+/-1.4 Gyr and [Z/H] = -0.79 +/- 0.04 dex, respectively, as well as [alpha/Fe] = 0.30 +/- 0.06. From the full spectral fitting technique, we measured a lower age (8.52 Gyr) and a similar total metallicity ([Z/H] = -0.86 dex). Conclusions. Our results indicate that NGC 5044-UCD1 is most likely an extreme GC (MV ~ -12.5 mag) belonging to the GC system of the elliptical galaxy NGC 5044.

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