Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00553784" target="_blank" >RIV/67985815:_____/22:00553784 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1051/0004-6361/202142791" target="_blank" >https://doi.org/10.1051/0004-6361/202142791</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/202142791" target="_blank" >10.1051/0004-6361/202142791</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud

Popis výsledku v původním jazyce

We report the detection of CO emission in the recently discovered multiphase isolated gas cloud in the nearby galaxy cluster Abell 1367. The cloud is located about 800 kpc in projection from the center of the cluster and at a projected distance of > 80 kpc from any galaxy. It is the first and the only known isolated “intra-cluster” cloud detected in X-ray, H alpha, and CO emission. We found a total of about 2.2 x 10(8)M(circle dot) of H-2 with the IRAM 30-m telescope in two regions, one associated with the peak of H alpha emission and another with the peak of X-ray emission surrounded by weak H alpha filaments. The velocity of the molecular gas is offset from the underlying H alpha emission by > 100 km s(-1) in the region where the X-ray peaks. The molecular gas may account for about 10% of the total cloud's mass, which is dominated by the hot X-ray component. The previously measured upper limit on the star formation rate in the cloud indicates that the molecular component is in a non-star-forming state, possibly due to a combination of low density of the gas and the observed level of velocity dispersion. The presence of the three gas phases associated with the cloud suggests that gas phase mixing with the surrounding intra-cluster medium is taking place. The possible origin of the orphan cloud is a late evolutionary stage of a ram pressure stripping event. In contrast, the nearby ram pressure stripped galaxy 2MASX J11443212+2006238 is in an early phase of stripping and we detected about 2.4 x 10(9)M(circle dot) of H-2 in its main body.

Název v anglickém jazyce

Non-star-forming molecular gas in the Abell 1367 intra-cluster multiphase orphan cloud

Popis výsledku anglicky

We report the detection of CO emission in the recently discovered multiphase isolated gas cloud in the nearby galaxy cluster Abell 1367. The cloud is located about 800 kpc in projection from the center of the cluster and at a projected distance of > 80 kpc from any galaxy. It is the first and the only known isolated “intra-cluster” cloud detected in X-ray, H alpha, and CO emission. We found a total of about 2.2 x 10(8)M(circle dot) of H-2 with the IRAM 30-m telescope in two regions, one associated with the peak of H alpha emission and another with the peak of X-ray emission surrounded by weak H alpha filaments. The velocity of the molecular gas is offset from the underlying H alpha emission by > 100 km s(-1) in the region where the X-ray peaks. The molecular gas may account for about 10% of the total cloud's mass, which is dominated by the hot X-ray component. The previously measured upper limit on the star formation rate in the cloud indicates that the molecular component is in a non-star-forming state, possibly due to a combination of low density of the gas and the observed level of velocity dispersion. The presence of the three gas phases associated with the cloud suggests that gas phase mixing with the surrounding intra-cluster medium is taking place. The possible origin of the orphan cloud is a late evolutionary stage of a ram pressure stripping event. In contrast, the nearby ram pressure stripped galaxy 2MASX J11443212+2006238 is in an early phase of stripping and we detected about 2.4 x 10(9)M(circle dot) of H-2 in its main body.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/LM2018106" target="_blank" >LM2018106: Atacama Large Millimeter/ Submillimeter Array – účast České republiky</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Astronomy & Astrophysics

ISSN

0004-6361

e-ISSN

1432-0746

Svazek periodika

658

Číslo periodika v rámci svazku

February

Stát vydavatele periodika

FR - Francouzská republika

Počet stran výsledku

6

Strana od-do

L5

Kód UT WoS článku

000751050500003

EID výsledku v databázi Scopus

2-s2.0-85124699004