Relativistic supernova 2009bb exploded close to an atomic gas cloud

M. J. Michałowski; G. Gentile; T. Krühler; H. Kuncarayakti; P. Kamphuis; J. Hjorth; S. Berta; V. D’Elia; J. Elliott; L. Galbany; J. Greiner; L. K. Hunt; M. P. Koprowski; E. Le Floc’h; A. Nicuesa Guelbenzu; E. Palazzi; J. Rasmussen; A. Rossi; S. Savaglio; A. de Ugarte Postigo; P. van der Werf; S. D. Vergani

doi:10.1051/0004-6361/201732356

Home

All issues

Volume 618 (October 2018)

A&A, 618 (2018) A104

Full HTML

Free Access

Table 2.

M AGPHYS results from the SED fitting.

logL_IR	SFR	sSFR	log M_*	log M_d	τ_V	T_cold	ξ_cold	T_warm	ξ_warm	ξ_hot	ξ_PAH	f_μ	log age_M
L_⊙)	(M_⊙ yr⁻¹)	(Gyr⁻¹)	(M_⊙)	(M_⊙)		(K)		(K)					(yr)
(¹)	(²)	(³)	(⁴)	(⁵)	(⁶)	(⁷)	(⁸)	(⁹)	(¹⁰)	(¹¹)	(¹²)	(¹³)	(¹⁴)

Notes.

⁽¹⁾

8−1000 μm infrared luminosity.

⁽²⁾

Star formation rate from SED modelling.

⁽³⁾

Specific star formation rate (≡SFR/M_*).

⁽⁴⁾

Stellar mass.

⁽⁵⁾

Dust mass.

⁽⁶⁾

Average V-band optical depth (A_V = 1.086τ_V).

⁽⁷⁾

Temperature of the cold dust component.

⁽⁸⁾

Contribution of the cold component to the infrared luminosity.

⁽⁹⁾

Temperature of the warm dust component.

⁽¹⁰⁾

Contribution of the warm component to the infrared luminosity.

⁽¹¹⁾

Contribution of the hot (130–250 K, mid-IR continuum) component to the infrared luminosity.

⁽¹²⁾

Contribution of the PAH component to the infrared luminosity.

⁽¹³⁾

Contribution of the ISM dust (as opposed to birth clouds) to the infrared luminosity.

⁽¹⁴⁾

Mass-weighted age.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.