A Snapshot Survey of Nearby Supernovae with the Hubble Space Telescope
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866929439309299712 |
|---|---|
| author | Baer-Way, Raphael DeGraw, Asia Zheng, Weikang Van Dyk, Schuyler D. Filippenko, Alexei V. Fox, Ori D. Brink, Thomas G. Kelly, Patrick L. Smith, Nathan Vasylyev, Sergiy S. de Jaeger, Thomas Zhang, Keto Stegman, Samantha Ross, Timothy Yunus, Sameen |
| author_facet | Baer-Way, Raphael DeGraw, Asia Zheng, Weikang Van Dyk, Schuyler D. Filippenko, Alexei V. Fox, Ori D. Brink, Thomas G. Kelly, Patrick L. Smith, Nathan Vasylyev, Sergiy S. de Jaeger, Thomas Zhang, Keto Stegman, Samantha Ross, Timothy Yunus, Sameen |
| contents | Over recent decades, robotic (or highly automated) searches for supernovae (SNe) have discovered several thousand events, many of them in quite nearby galaxies (distances < 30 Mpc). Most of these SNe, including some of the best-studied events to date, were found before maximum brightness and have associated with them extensive follow-up photometry and spectroscopy. Some of these discoveries are so-called SN impostors, thought to be superoutbursts of luminous blue variable stars, although possibly a new, weak class of massive-star explosions. We conducted a Snapshot program with the Hubble Space Telescope(HST) and obtained images of the sites of 31 SNe and four impostors, to acquire late-time photometry through two filters. The primary aim of this project was to reveal the origin of any lingering energy for each event, whether it is the result of radioactive decay or, in some cases, ongoing late-time interaction of the SN shock with pre-existing circumstellar matter, or the presence of a light echo. Alternatively, lingering faint light at the SN position may arise from an underlying stellar population (e.g., a host star cluster, companion star, or a chance alignment). The results from this study complement and extend those from Snapshot programs by various investigators in previous HST cycles. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_12185 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A Snapshot Survey of Nearby Supernovae with the Hubble Space Telescope Baer-Way, Raphael DeGraw, Asia Zheng, Weikang Van Dyk, Schuyler D. Filippenko, Alexei V. Fox, Ori D. Brink, Thomas G. Kelly, Patrick L. Smith, Nathan Vasylyev, Sergiy S. de Jaeger, Thomas Zhang, Keto Stegman, Samantha Ross, Timothy Yunus, Sameen High Energy Astrophysical Phenomena Over recent decades, robotic (or highly automated) searches for supernovae (SNe) have discovered several thousand events, many of them in quite nearby galaxies (distances < 30 Mpc). Most of these SNe, including some of the best-studied events to date, were found before maximum brightness and have associated with them extensive follow-up photometry and spectroscopy. Some of these discoveries are so-called SN impostors, thought to be superoutbursts of luminous blue variable stars, although possibly a new, weak class of massive-star explosions. We conducted a Snapshot program with the Hubble Space Telescope(HST) and obtained images of the sites of 31 SNe and four impostors, to acquire late-time photometry through two filters. The primary aim of this project was to reveal the origin of any lingering energy for each event, whether it is the result of radioactive decay or, in some cases, ongoing late-time interaction of the SN shock with pre-existing circumstellar matter, or the presence of a light echo. Alternatively, lingering faint light at the SN position may arise from an underlying stellar population (e.g., a host star cluster, companion star, or a chance alignment). The results from this study complement and extend those from Snapshot programs by various investigators in previous HST cycles. |
| title | A Snapshot Survey of Nearby Supernovae with the Hubble Space Telescope |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2401.12185 |