Abstract
We present a low-redshift (z = 0.029) damped Lyα (DLA) system in the spectrum of a background quasi-stellar object (QSO). The DLA is associated with an interacting galaxy pair within a galaxy group. We detected weak Lyα emission centered at the absorption trough of the DLA. The emission was likely tracing the neutral H i reservoir around the galaxies in the interacting pair, which scattered the Lyα generated by star formation within those galaxies. We also found that the interacting pair is enveloped by a large H i cloud with . We discovered blueshifted 21 cm H i emission, corresponding to M(H i) = , associated with J151225.15+012950.4 - one of the galaxies in the interacting pair. The blueshifted H i was tracing gas flowing into the galaxy from behind and toward us. Gas at similar blueshifted velocities was seen in the QSO sight line, thus suggesting the presence of a filamentary structure of the order of 100 kpc feeding the galaxy. We estimated a mass inflow rate of into the galaxy, which matches the star formation rate estimated from Hα emission. It is likely that the inflow of enormous amounts of gas has triggered star formation in this galaxy. The sudden acquisition of cold gas may lead to a starburst in this galaxy like those commonly seen in simulations.
| Original language | English (US) |
|---|---|
| Article number | 239 |
| Journal | Astrophysical Journal |
| Volume | 871 |
| Issue number | 2 |
| DOIs | |
| State | Published - Feb 1 2019 |
Fingerprint
Keywords
- galaxies: halos
- galaxies: ISM
- galaxies: starburst
- quasars: absorption lines
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Cite this
Discovery of a Damped Lyα System in a Low-z Galaxy Group : Possible Evidence for Gas Inflow and Nuclear Star Formation. / Borthakur, Sanchayeeta; Momjian, Emmanuel; Heckman, Timothy M.; Catinella, Barbara; Vogt, Frédéric P.A.; Tumlinson, Jason.
In: Astrophysical Journal, Vol. 871, No. 2, 239, 01.02.2019.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Discovery of a Damped Lyα System in a Low-z Galaxy Group
T2 - Possible Evidence for Gas Inflow and Nuclear Star Formation
AU - Borthakur, Sanchayeeta
AU - Momjian, Emmanuel
AU - Heckman, Timothy M.
AU - Catinella, Barbara
AU - Vogt, Frédéric P.A.
AU - Tumlinson, Jason
PY - 2019/2/1
Y1 - 2019/2/1
N2 - We present a low-redshift (z = 0.029) damped Lyα (DLA) system in the spectrum of a background quasi-stellar object (QSO). The DLA is associated with an interacting galaxy pair within a galaxy group. We detected weak Lyα emission centered at the absorption trough of the DLA. The emission was likely tracing the neutral H i reservoir around the galaxies in the interacting pair, which scattered the Lyα generated by star formation within those galaxies. We also found that the interacting pair is enveloped by a large H i cloud with . We discovered blueshifted 21 cm H i emission, corresponding to M(H i) = , associated with J151225.15+012950.4 - one of the galaxies in the interacting pair. The blueshifted H i was tracing gas flowing into the galaxy from behind and toward us. Gas at similar blueshifted velocities was seen in the QSO sight line, thus suggesting the presence of a filamentary structure of the order of 100 kpc feeding the galaxy. We estimated a mass inflow rate of into the galaxy, which matches the star formation rate estimated from Hα emission. It is likely that the inflow of enormous amounts of gas has triggered star formation in this galaxy. The sudden acquisition of cold gas may lead to a starburst in this galaxy like those commonly seen in simulations.
AB - We present a low-redshift (z = 0.029) damped Lyα (DLA) system in the spectrum of a background quasi-stellar object (QSO). The DLA is associated with an interacting galaxy pair within a galaxy group. We detected weak Lyα emission centered at the absorption trough of the DLA. The emission was likely tracing the neutral H i reservoir around the galaxies in the interacting pair, which scattered the Lyα generated by star formation within those galaxies. We also found that the interacting pair is enveloped by a large H i cloud with . We discovered blueshifted 21 cm H i emission, corresponding to M(H i) = , associated with J151225.15+012950.4 - one of the galaxies in the interacting pair. The blueshifted H i was tracing gas flowing into the galaxy from behind and toward us. Gas at similar blueshifted velocities was seen in the QSO sight line, thus suggesting the presence of a filamentary structure of the order of 100 kpc feeding the galaxy. We estimated a mass inflow rate of into the galaxy, which matches the star formation rate estimated from Hα emission. It is likely that the inflow of enormous amounts of gas has triggered star formation in this galaxy. The sudden acquisition of cold gas may lead to a starburst in this galaxy like those commonly seen in simulations.
KW - galaxies: halos
KW - galaxies: ISM
KW - galaxies: starburst
KW - quasars: absorption lines
UR - http://www.scopus.com/inward/record.url?scp=85062012510&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85062012510&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/aaf566
DO - 10.3847/1538-4357/aaf566
M3 - Article
AN - SCOPUS:85062012510
VL - 871
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
M1 - 239
ER -