# HST resolves stars in a tiny body falling on the dwarf galaxy DDO 68

**Authors:** F. Annibali (1), M. Bellazzini (1), M. Correnti (2), E. Sacchi (2), M., Tosi (1), M. Cignoni (3), A. Aloisi (2), D. Calzetti (4), L. Ciotti (5), F., Cusano (1), J. Lee (6), C. Nipoti (5) ((1) INAF-Astrophysics, Space, Science Observatory, Bologna, Italy (2) Space Telescope Science Institute,, Baltimore, USA (3) Dipartimento di Fisica, Universita' di Pisa, Italy (4), Department of Astronomy, University of Massachusetts-Amherst, USA (5), Dipartimento di Fisica e Astronomia, Universita' di Bologna, Italy (6), Caltech-IPAC, USA)

arXiv: 1904.01986 · 2019-09-25

## TL;DR

HST imaging reveals a star stream associated with dwarf galaxy DDO 68, showing old stars and evidence of hierarchical merging at the dwarf galaxy scale.

## Contribution

First resolved imaging of a star stream in a dwarf galaxy, confirming its association with DDO 68 and providing insights into its star formation history.

## Key findings

- Stream contains predominantly old RGB stars.
- Star formation in the stream ceased over 1 Gyr ago.
- Stream's stellar mass is about 1% of DDO 68's mass.

## Abstract

We present new Hubble Space Telescope (HST) imaging of a stream-like system associated with the dwarf galaxy DDO 68, located in the Lynx-Cancer Void at a distance of D$\sim$12.65 Mpc from us. The stream, previously identified in deep Large Binocular Telescope images as a diffuse low surface brightness structure, is resolved into individual stars in the F606W (broad V) and F814W ($\sim$I) images acquired with the Wide Field Camera 3. The resulting V, I color-magnitude diagram (CMD) of the resolved stars is dominated by old (age$\gtrsim$1-2 Gyr) red giant branch (RGB) stars. From the observed RGB tip, we conclude that the stream is at the same distance as DDO 68, confirming the physical association with it. A synthetic CMD analysis indicates that the large majority of the star formation activity in the stream occurred at epochs earlier than $\sim$1 Gyr ago, and that the star formation at epochs more recent than $\sim$500 Myr ago is compatible with zero. The total stellar mass of the stream is $\sim10^{6} M_{\odot}$, about 1/100 of that of DDO~68. This is a striking example of hierarchical merging in action at the dwarf galaxy scales.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1904.01986/full.md

## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1904.01986/full.md

## References

55 references — full list in the complete paper: https://tomesphere.com/paper/1904.01986/full.md

---
Source: https://tomesphere.com/paper/1904.01986